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X-WR-CALDESC:Eventi per Osservatorio Astronomico di Roma
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DTSTART:20180325T010000
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DTSTART:20230326T010000
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DTSTART:20231029T010000
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END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20220125T113000
DTEND;TZID=Europe/Rome:20220125T123000
DTSTAMP:20260404T205326
CREATED:20220119T145638Z
LAST-MODIFIED:20220119T145638Z
UID:10265-1643110200-1643113800@www.oa-roma.inaf.it
SUMMARY:colloquium Anita Zanella: The contribution of high-redshift star-forming regions to galaxy evolution
DESCRIPTION:Observations have shown that local galaxies have modest star formation rates and form the bulk of their stars in giant molecular clouds. In comparison\, galaxies in the early Universe have high star formation rates and host large star-forming regions (dubbed “clumps”)\, 10 – 1000 times larger\, brighter\, and more massive than local giant molecular clouds. Interestingly\, the formation phase of clumps has rarely been observed and their fate is highly uncertain. Are they born in-situ due to fragmentation of gas-rich disks or are they small satellite galaxies that merged with the host? Do they migrate inward and contribute to the formation of the galaxy bulge or are they rapidly disrupted by stellar feedback? Do they play a role in the mass assembly and structural evolution of the host galaxy? I will discuss our latest results derived from spatially-resolved HST\, VLT/MUSE and ALMA datasets\, as well as mock observations created from hydrodynamical simulations\, which provide some answers to these open questions. \n\n\n 
URL:https://www.oa-roma.inaf.it/event/colloquium-anita-zanella-the-contribution-of-high-redshift-star-forming-regions-to-galaxy-evolution/
LOCATION:RM
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20210126T113000
DTEND;TZID=Europe/Rome:20210126T123000
DTSTAMP:20260404T205326
CREATED:20201219T111234Z
LAST-MODIFIED:20201219T111234Z
UID:8753-1611660600-1611664200@www.oa-roma.inaf.it
SUMMARY:colloquium - Michele Fabrizio
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-michele-fabrizio/
LOCATION:RM
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20210119T113000
DTEND;TZID=Europe/Rome:20210119T123000
DTSTAMP:20260404T205326
CREATED:20201219T111134Z
LAST-MODIFIED:20201219T111134Z
UID:8751-1611055800-1611059400@www.oa-roma.inaf.it
SUMMARY:colloquium - Flavia Dell'Agli
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-flavia-dellagli-2/
LOCATION:RM
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20210113T113000
DTEND;TZID=Europe/Rome:20210113T123000
DTSTAMP:20260404T205326
CREATED:20201219T105808Z
LAST-MODIFIED:20201219T110954Z
UID:8749-1610537400-1610541000@www.oa-roma.inaf.it
SUMMARY:The X-ray rise of primeval titans: HYPerluminous quasars at the Epoch of ReionizatION (HYPERION)
DESCRIPTION:The outstanding mass growth of the Supermassive Black Holes powering\nluminous quasars at the Epoch of Reionization (EoR\, z > 6) is one of\nthe most debated open problems of modern extragalactic\nastrophysics. These quasars are current targets of extensive\nmultiwavelength campaigns with todays flagship observatories\, in order\nto understand their properties. The limited sensitivity of current\nX-ray observatories\, however\, has so far provided mostly low quality\nspectra (< 10 − 15 counts; 0.5-10 keV) and therefore a poor\ncharacterization of their nuclear properties. I will present HYPERION\,\na 2.4 Ms Multi-Year Heritage XMM programme on the titans among z = 6 −\n7.5 quasars (i.e. the most luminous/massive at their epoch) designed\nto dramatically improve the X-ray data quality to 100 counts for a\nsample of 15 sources. HYPERION will deliver unprecedented constraints\non their nuclear properties\, accretion\, ejection\, disc/corona complex\,\nand\, while perfectly complementing observations at other wavelengths\,\nwill enable X-ray spectroscopic population studies at EoR to begin.
URL:https://www.oa-roma.inaf.it/event/the-x-ray-rise-of-primeval-titans-hyperluminous-quasars-at-the-epoch-of-reionization-hyperion/
LOCATION:RM
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200505T114500
DTEND;TZID=Europe/Rome:20200505T124500
DTSTAMP:20260404T205326
CREATED:20191031T060837Z
LAST-MODIFIED:20200121T150815Z
UID:7034-1588679100-1588682700@www.oa-roma.inaf.it
SUMMARY:colloquium - Hans Van Winckel
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-hans-van-winckel/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200428T114500
DTEND;TZID=Europe/Rome:20200428T124500
DTSTAMP:20260404T205326
CREATED:20200131T083054Z
LAST-MODIFIED:20200131T163718Z
UID:7374-1588074300-1588077900@www.oa-roma.inaf.it
SUMMARY:colloquium - Suzanne Ramsey
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-suzan-ramsey/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200420T114500
DTEND;TZID=Europe/Rome:20200420T124500
DTSTAMP:20260404T205326
CREATED:20191211T154418Z
LAST-MODIFIED:20200113T110038Z
UID:7208-1587383100-1587386700@www.oa-roma.inaf.it
SUMMARY:colloquium - Giovanni Miniutti
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-giovanni-miniutti/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200407T114500
DTEND;TZID=Europe/Rome:20200407T124500
DTSTAMP:20260404T205326
CREATED:20191113T105052Z
LAST-MODIFIED:20191113T105052Z
UID:7085-1586259900-1586263500@www.oa-roma.inaf.it
SUMMARY:colloquium - Matt Middleton
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-matt-middleton/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200324T114500
DTEND;TZID=Europe/Rome:20200324T124500
DTSTAMP:20260404T205326
CREATED:20200117T082551Z
LAST-MODIFIED:20200117T082551Z
UID:7290-1585050300-1585053900@www.oa-roma.inaf.it
SUMMARY:colloquium - Eleonora Fiorellino
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-eleonora-fiorellino/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200317T114500
DTEND;TZID=Europe/Rome:20200317T124500
DTSTAMP:20260404T205326
CREATED:20200110T123928Z
LAST-MODIFIED:20200110T123928Z
UID:7272-1584445500-1584449100@www.oa-roma.inaf.it
SUMMARY:colloquium - Brian Chaboyer
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-brian-chaboyer/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200310T114500
DTEND;TZID=Europe/Rome:20200310T124500
DTSTAMP:20260404T205326
CREATED:20200121T150505Z
LAST-MODIFIED:20200121T150505Z
UID:7311-1583840700-1583844300@www.oa-roma.inaf.it
SUMMARY:The role of starburst galaxies and mergers in the distant Universe
DESCRIPTION:Starburst galaxies are the most luminous star-forming powered objects in the Universe. A long standing problem in galaxy evolution is to understand whether these systems are caused by merger events\, or they are just gas rich galaxies undergoing stochastic accretion events. To properly characterize them\, we need infrared data\, given the huge dust attenuations affecting their UV and optical emission. \nI will present a unique set of near-infrared rest-frame spectral observations of star-forming galaxies at redshift ~ 0.7\, and show how these can be used to understand the dust properties and origin of starbursts. Furthermore\, I will explain how additional multiwavelength information (from radio to X-rays) is crucial to trace the whole sequence of mergers\, test the merger-AGN connection and the formation mechanism of passive galaxies. Finally\, I will exploit high-resolution HST images to investigate the role of mergers on the origin of bright star-forming clumps in high-redshift galaxies. A complete study of near-infrared rest-frame lines will allow JWST to probe the physical properties (e.g.\, dust attenuation\, metallicity) and the nature of the most dust-embedded systems up to the reionization epoch.
URL:https://www.oa-roma.inaf.it/event/the-role-of-starburst-galaxies-and-mergers-in-the-distant-universe/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200303T114500
DTEND;TZID=Europe/Rome:20200303T124500
DTSTAMP:20260404T205326
CREATED:20200117T082906Z
LAST-MODIFIED:20200117T082906Z
UID:7292-1583235900-1583239500@www.oa-roma.inaf.it
SUMMARY:colloquium - Ester Marini
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-ester-marini/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200228T114500
DTEND;TZID=Europe/Rome:20200228T124500
DTSTAMP:20260404T205326
CREATED:20191016T143241Z
LAST-MODIFIED:20200127T143943Z
UID:6932-1582890300-1582893900@www.oa-roma.inaf.it
SUMMARY:colloquium - Roberta Zanin
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-roberta-zanin/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200218T114500
DTEND;TZID=Europe/Rome:20200218T124500
DTSTAMP:20260404T205326
CREATED:20190723T115244Z
LAST-MODIFIED:20200207T102810Z
UID:6539-1582026300-1582029900@www.oa-roma.inaf.it
SUMMARY:The interstellar medium at high redshift
DESCRIPTION:The gaseous content of galaxies is one of the key ingredients of galaxy evolution: It fuels star formation and nuclear activity\, and at the same time it is the main receiver of any feedback mechanism from these two processes. However\, we have only very limited knowledge of the gas content and of its physical properties in galaxies beyond the local universe. As a result\, no description of galaxy formation can be fully validated without a better understanding of 1) how much gas was available for star formation in different cosmic times; 2) how the star formation efficiency\, i.e.\, the capability of a galaxy to form stars from a given amount of gas\, evolve through cosmic history\, and which are physical conditions that governed this evolution; 3) what was the interplay between the interstellar medium\, star formation\, and nuclear activity. These questions are particularly critical at the very high redshifts (z>6\, when the universe was <1 Gyr old)\, where our census of galaxies is highly incomplete\, especially at the high-mass end\, and galaxies followed very different evolution according to the mass of their initial gas reservoir. In this talk I will present the results of various observational campaigns aimed at addressing these questions\, in particular by capitalizing on the unprecedented capabilities offered by the Atacama Large Millimeter Array and the Northern Extended Millimeter Array. These findings will guide the next generation of simulations and theoretical models\, thus marking a transformational step in our understanding of galaxy evolution.
URL:https://www.oa-roma.inaf.it/event/roberto-de-carli-colloquium/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200211T114500
DTEND;TZID=Europe/Rome:20200211T124500
DTSTAMP:20260404T205326
CREATED:20191018T072026Z
LAST-MODIFIED:20200122T132159Z
UID:6942-1581421500-1581425100@www.oa-roma.inaf.it
SUMMARY:The quest for observational evidence of the hierarchical formation process at the smallest galaxy scales
DESCRIPTION:I will present our ongoing project devoted to the search and study of satellites\, stellar streams\, and substructures around dwarf galaxies. Deep\, wide field imaging acquired with the Large Binocular Telescope and follow-up observations performed with the WFC3 on the Hubble Space Telescope provide evidence of multiple satellites associated with the very metal-poor star-forming dwarf galaxy DDO 68. This is a striking example of the few observed cases of hierarchical merging in action at the dwarf galaxy scales. To perform a systematic search of substructures around dwarf galaxies\, we have started a Strategic Program at the LBT\, named SSH (i.e. The Smallest Scales of Hierarchy Survey) to acquire deep\, wide-field imaging of a sample of 45 late-type dwarf galaxies located within 10 Mpc. The survey\, which is now close to completion\, will provide one of the first systematic observational studies of the hierarchical formation process down to very small galaxy scales. In this talk I will introduce SSH and discuss the results obtained so far.
URL:https://www.oa-roma.inaf.it/event/colloquium-francesca-annibali/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200204T114500
DTEND;TZID=Europe/Rome:20200204T124500
DTSTAMP:20260404T205326
CREATED:20190926T124553Z
LAST-MODIFIED:20200127T150346Z
UID:6853-1580816700-1580820300@www.oa-roma.inaf.it
SUMMARY:The X-ray universe at microarsec resolution: the power and promise of X-ray interferometry
DESCRIPTION:The spectacular image of a supermassive black hole `shadow’ taken by the Event Horizon Telescope last year highlights the potential of being able to resolve microarcsecond scale structures in astrophysical sources.  Given the ~Angstrom scale of X-ray wavelengths\, similar resolutions are theoretically possible with only a 1 m diameter telescope\, which could be accommodated on a single spacecraft. Conventional X-ray imaging capability remains far from from this goal however.\nIn this talk I will explore the possibility\, recently proposed to ESA’s Voyage 2050 program\, of developing X-ray interferometry to break the resolution barrier in the X-rays\, starting from X-ray fringes which have already been observed in the lab and examining what would be required for an X-ray interferometric space observatory\, from the possibilities with single spacecraft to formation flyers which could push to sub-microarcsecond resolution. Such revolutionary observatories would enable detailed imaging-spectroscopy of stellar coronae and transiting exoplanets within ~100 pc\, direct observation of X-ray binary orbits\, supermassive black hole accretion flows and event horizons\, and imaging of luminous transients and binary supermassive black holes across the observable universe.
URL:https://www.oa-roma.inaf.it/event/colloquium-phil-uttley/
LOCATION:OAR Monte Porzio Catone – aula Gratton\, Via Frascati 33\, Roma\, RM\, 00136\, Italia
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200128T114500
DTEND;TZID=Europe/Rome:20200128T124500
DTSTAMP:20260404T205326
CREATED:20191211T055526Z
LAST-MODIFIED:20191220T064506Z
UID:7190-1580211900-1580215500@www.oa-roma.inaf.it
SUMMARY:3D magnetic structure\, and brightening in sunspot penumbra
DESCRIPTION:We analyzed spectropolarimetric data in the Fe I 617.3 nm and Ca II 854.2 nm lines of the sunspot in AR 12546 observed with the IBIS at the Dunn Solar Telescope on 20th May 2016 and co-temporal filtergrams by space-borne (Hinode\, IRIS and SDO) instruments. The observed sunspot is one among the largest such features occurred over the last solar cycle. The IBIS data\, taken under excellent seeing conditions that lasted more than three hours\, were inverted with the NICOLE code\, in order to retrieve the temperature\, magnetic field\, and plasma velocity of the studied sunspot as a function of optical depth and time. The umbral and penumbral regions are for the most part stable in the photosphere\, while co-spatial chromospheric areas show waves in the umbra-penumbra boundary and intense brightening along penumbral filaments. We explored the origin of these chromospheric processes and their relation to changes in the 3D magnetic structure of the observed sunspot.
URL:https://www.oa-roma.inaf.it/event/colloquium-mariarita-murabito/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200121T114500
DTEND;TZID=Europe/Rome:20200121T124500
DTSTAMP:20260404T205326
CREATED:20191009T121842Z
LAST-MODIFIED:20191009T121842Z
UID:6909-1579607100-1579610700@www.oa-roma.inaf.it
SUMMARY:colloquium - Matteo Bachetti
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/colloquium-matteo-bachetti/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20200114T114500
DTEND;TZID=Europe/Rome:20200114T124500
DTSTAMP:20260404T205326
CREATED:20191008T060530Z
LAST-MODIFIED:20200107T140305Z
UID:6889-1579002300-1579005900@www.oa-roma.inaf.it
SUMMARY:The two-families scenario: what does it predict?
DESCRIPTION:I will revisit the two-families scenario in which neutron stars coexist with strange quark stars\, i.e. with compact objects made almost\nentirely of deconfined quarks. I will outline the differences between this scenario and other schemes in which quark matter appears only at the center of compact stars and I will discuss how it compares with GW170817\, GRB170817A\, AT2017gfo and with the existing limits on masses and radii of compact stars.
URL:https://www.oa-roma.inaf.it/event/colloquium-alessandro-drago/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191218T114500
DTEND;TZID=Europe/Rome:20191218T124500
DTSTAMP:20260404T205326
CREATED:20191201T160620Z
LAST-MODIFIED:20191212T083130Z
UID:7142-1576669500-1576673100@www.oa-roma.inaf.it
SUMMARY:Gamma-ray bursts under a new light: the TeV emission from GRB190114C seen by the MAGIC telescopes
DESCRIPTION:Gamma-ray bursts (GRBs) are the most luminous sources of electromagnetic radiation known in the Universe. GRBs had been observed over a broad energy range from the radio band up to GeV gamma rays\, but the TeV gamma-ray band had remained terra incognita for a long time. Thanks to the MAGIC telescopes\, designed to catch the fast glimpses of the GRBs\, the first ever clear detection in this band was achieved for GRB 190114C\, a bright\, long GRB. The TeV emission from GRB190114C belongs to a new energetic component\, providing an energy output comparable at the one at lower energies. We will discuss the details of the observations by MAGIC and the accompanying multi-frequency measurements by more than 20 instruments\, from radio to gamma- rays\, and the inferences on the emission mechanisms. This historical\, highly significant detection has followed an intriguing hint of TeV emission from GRB 160821B\, a short GRB with an associated kilonova. This hint\, if real\, has potential multi-messenger implications on the detectability of gravitational wave alerts in high-energy gamma-rays. \n 
URL:https://www.oa-roma.inaf.it/event/colloquium-antonio-stamerra-3/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191210T114500
DTEND;TZID=Europe/Rome:20191210T124500
DTSTAMP:20260404T205326
CREATED:20190723T112945Z
LAST-MODIFIED:20191204T155611Z
UID:6537-1575978300-1575981900@www.oa-roma.inaf.it
SUMMARY:Characterizing multi-phase gas outflows and their powering mechanism in nearby AGN
DESCRIPTION:Active Galactic Nuclei are thought to play a crucial role in\nthe evolution of massive galaxies. In particular\, fast outflows are\nfrequently observed in AGN covering various gas phases which may remove\na significant fraction of the gas content from the galaxies. I will\nreview the current state of research in this very active field of\nongoing research together with the advantages and disadvantages of\nprevious approaches. In particular\, I will highlight the importance of\nmulti-wavelength observations to unravel the true multi-phase nature of\noutflows by combining state-of-the-art observational facilities. In this\ncontext I will present the first results from the ongoing Close AGN\nReference Survey (CARS)\, a multi-wavelength survey of 39 luminous\nlow-redshift unobscured AGN with extensive observations from VLT/MUSE\,\nALMA\, VLA\, Chandra\, SOFIA and many more. In addition\, I will present the\nmulti-phase view of the famous ultra-luminous Quasar 3C273 where we\nunlocked a few unknown secrets.
URL:https://www.oa-roma.inaf.it/event/colloquium-bernd-husemann/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191203T114500
DTEND;TZID=Europe/Rome:20191203T124500
DTSTAMP:20260404T205326
CREATED:20190723T160231Z
LAST-MODIFIED:20191201T160753Z
UID:6544-1575373500-1575377100@www.oa-roma.inaf.it
SUMMARY:Acoustic oscillations and dynamo action in giants
DESCRIPTION:The role of the magnetic field in determining the angular momentum  transport in stellar interior is still an open issue. Acoustic oscillations are directly affected by the presence of a large-scale magnetic field but their study can provide fundamental information on the properties of the magnetic fields in solar-like stars. As an example the case of  EK Eridani\, a slowly rotating\, overactive G8 giant\, will be presented.  Moreover the possibility to use asteroseismology to solve the  long-lasting mystery on the origin of magnetic fields in Ap stars will be discussed.
URL:https://www.oa-roma.inaf.it/event/alfio-bonanno-colloquium/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191126T114500
DTEND;TZID=Europe/Rome:20191126T124500
DTSTAMP:20260404T205326
CREATED:20190919T100822Z
LAST-MODIFIED:20191123T102647Z
UID:6767-1574768700-1574772300@www.oa-roma.inaf.it
SUMMARY:LSST: an opportunity for the Italian Community
DESCRIPTION:We review the current status of the LSST project\, its expected performances\, the key science goals and the involvment of the Italian Community
URL:https://www.oa-roma.inaf.it/event/colloquium-giuliana-fiorentino/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191125T080000
DTEND;TZID=Europe/Rome:20191128T170000
DTSTAMP:20260404T205326
CREATED:20191122T181336Z
LAST-MODIFIED:20191122T181336Z
UID:7116-1574668800-1574960400@www.oa-roma.inaf.it
SUMMARY:workshop Stamerra
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/workshop-stamerra/
LOCATION:Aula Gratton
CATEGORIES:Congressi
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191118T090000
DTEND;TZID=Europe/Rome:20191122T180000
DTSTAMP:20260404T205326
CREATED:20190111T102035Z
LAST-MODIFIED:20190111T102139Z
UID:5155-1574067600-1574445600@www.oa-roma.inaf.it
SUMMARY:Lithium in the Universe: to Be or not to Be
DESCRIPTION:
URL:https://www.oa-roma.inaf.it/event/lithium-in-the-universe-to-be-or-not-to-be/
LOCATION:OAR Monte Porzio Catone – aula Gratton\, Via Frascati 33\, Roma\, RM\, 00136\, Italia
CATEGORIES:Congressi
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191115T160000
DTEND;TZID=Europe/Rome:20191115T170000
DTSTAMP:20260404T205326
CREATED:20191108T072725Z
LAST-MODIFIED:20191108T075652Z
UID:7070-1573833600-1573837200@www.oa-roma.inaf.it
SUMMARY:Dal Sole a Sedna: una passeggiata per il sistema solare\, e uno sguardo più in là
DESCRIPTION:Dal 1959 ad oggi più di cento sonde spaziali hanno lasciato la Terra verso la Luna e lo spazio profondo. Queste appendici robotica dei nostri sensi hanno visitato tutti i pianeti e i principali satelliti del sistema solare\, rivelando una straordinaria e inattesa varietà di forme e fenomeni. Ripercorrere vent’anni di scoperte sarà un tributo all’ingegno di quanti le hanno rese possibili. Grazie alle immagini più belle raccolte negli ultimi anni\, la conferenza ripercorrerà le scoperte più significative nell’esplorazione del sistema solare\, gettando infine uno sguardo ai pianeti delle stelle vicine. Forse tra questi ne esiste qualcuno che ospita la vita? Come trovarlo?
URL:https://www.oa-roma.inaf.it/event/dal-sole-a-sedna-una-passeggiata-per-il-sistema-solare-e-uno-sguardo-piu-in-la/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191114T114500
DTEND;TZID=Europe/Rome:20191114T124500
DTSTAMP:20260404T205326
CREATED:20191023T064535Z
LAST-MODIFIED:20191031T064029Z
UID:7011-1573731900-1573735500@www.oa-roma.inaf.it
SUMMARY:Lithium in the local Volume
DESCRIPTION:We present our recent study on the chemical evolution of lithium in the thin disc of the Milky Way.\nWe found that the best agreement with the observed Li abundances in the thin disc is obtained\nconsidering novae as the main source of lithium. We assumed a delay time of ≈1 Gyr  for nova\nproduction and an effective 7Li yield of 1.8(± 0.6)×10−5 Msun over the whole nova lifetime.\nThe possibility to check our detailed assumptions on lithium production on other stellar systems\, such\nas the satellites of our Milky Way\, is seriously hampered by their distance from us. In these  systems\ndwarf stars (where the original lithium can be measured) are too faint to detect lithium lines.\nHowever\, thanks to the Gaia mission\, it was recently possible to disentangle the stars of a disrupted\ndwarf galaxy in the Galactic halo (called Enceladus or Galactic sausage). Adopting a chemical evolution\nmodel able to match the chemical enrichment in alpha elements and the metallicity distribution function\nof Enceladus\, we present our prediction for the lithium abundance of the stars of this disrupted galaxy.
URL:https://www.oa-roma.inaf.it/event/colloquium-gabriele-cescutti/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191108T114500
DTEND;TZID=Europe/Rome:20191108T124500
DTSTAMP:20260404T205326
CREATED:20191105T085225Z
LAST-MODIFIED:20191105T085225Z
UID:7038-1573213500-1573217100@www.oa-roma.inaf.it
SUMMARY:The ultraluminous X-ray pulsar NGC 5907 ULX-1 and its nebula
DESCRIPTION:Ultraluminous X-ray pulsars are accretion-powered pulsars whose X-ray\nluminosity\, if isotropic\, largely exceeds their Eddington limit. Only a handful\nare known to date and NGC 5907 ULX-1\, distant 17 Mpc from us\, is the most luminous of them\,\nat 1e41 erg/s 500 times its Eddington limit. We constrained through\npulsar timing its orbit and spin behavior\, estimating a 5d orbital period and a spin-up\ntime <40 yr. We detected an extended X-ray feature surrounding the source: likely a young and\npowerful bubble driven by the wind from the accreting pulsar system. The nebula\nhas been powered at ~1e41 erg/s for ~70 kyr proving that a highly super-Eddington\nregime can be sustained for much longer than the spin-up time of the pulsar.\nI will present the current status of the observations and understanding of this system\nand the prospects to solve the still open problems it raises.
URL:https://www.oa-roma.inaf.it/event/the-ultraluminous-x-ray-pulsar-ngc-5907-ulx-1-and-its-nebula/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191105T114500
DTEND;TZID=Europe/Rome:20191105T124500
DTSTAMP:20260404T205326
CREATED:20191016T061058Z
LAST-MODIFIED:20191030T155258Z
UID:6926-1572954300-1572957900@www.oa-roma.inaf.it
SUMMARY:The impact of AGB stars on the life of stellar systems
DESCRIPTION:During the latest phases of their lives\, low-intermediate mass stars (M<8Msun) evolve through the Asymptotic Giant branch (AGB) phase. Although very rapid\, the AGB phase represents a crucial step for the chemical evolution of the system where these stars form. The reason is that AGB stars undergo an advanced nucleosynthesis and experiment dredge-up events\, while they progressively lose the majority of their mass through stellar winds. Furthermore\, the low temperature and high densisty of their stellar winds prove extremely favourable conditions for dust condensation in the circumstellar envelopes. All the reprocessed gas and dust lost by the AGB stars enrich the insterstellar medium of the host system. Detailed modelling of these complex physical processes are essential to reconstruct the impact that these stars had on the history of formation and chemical evolution of stellar clusters and galaxies. In this talk I will present how the latest generation of AGB+dust evolutionary models has been recently used to this scope in different environments: from globular clusters\, to unveil the origine of multiple populations\, to Local Group dwarf galaxies\, to infer star formation history and dust production rate.
URL:https://www.oa-roma.inaf.it/event/colloquium-flavia-dellagli/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20191029T114500
DTEND;TZID=Europe/Rome:20191029T124500
DTSTAMP:20260404T205326
CREATED:20191020T043613Z
LAST-MODIFIED:20191020T043613Z
UID:6990-1572349500-1572353100@www.oa-roma.inaf.it
SUMMARY:Post-AGB stars as tracers of the origin of elements in the Universe
DESCRIPTION:The chemical evolution of galaxies is governed by the chemical yields from stars\, especially from Asymptotic Giant Branch (AGB) stars. This underlines the importance of understanding how AGB stars produce their elements by obtaining accurate stellar nucleosynthetic yields. Although AGB nucleosynthesis has general validity\, critical uncertainties (such as the treatment of convective-driven mixing processes and mass loss) exist in current stellar models. Observations from Post-Asymptotic Giant Branch (post-AGB) stars serve as excellent tools to confront predictions from a dedicated suite of stellar models\, quantify the strongest discrepancies\, and eliminate crucial uncertainties that hamper stellar modelling. Our recent studies of post-AGB stars have shown an intriguing chemical diversity that ranges from stars that are extremely enriched in carbon and s-process elements to the discovery of the first post-AGB star with no traces of carbon nor s-process elements. Additionally\, our studies have also shown that AGB nucleosynthesis is significantly affected by a binary companion. These results reflect the complexity that surrounds the element production in AGB stars. In this talk\, I will present the intriguing chemical diversity observed in post-AGB stars and its implications on element/isotope production in AGB stars and stellar nucleosynthetic yields.
URL:https://www.oa-roma.inaf.it/event/post-agb-stars-as-tracers-of-the-origin-of-elements-in-the-universe/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
END:VCALENDAR