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febbraio 2017

The challenge of massive black hole binary coalescence; from galaxy formation to gravitational waves

febbraio 21 @ 11:45 - 12:45 - Oratore: Lucio Mayer (Università di Zurigo)

I will review recent progress in understanding how a pair of massive black holes can…

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AGB dust production: what we learn from the Local Group galaxies

febbraio 28 @ 11:45 - 12:45 - Oratore: Flavia Dell'Agli (IAC - Tenerife)

Asymptotic giant branch (AGB) stars are among the most important gas and dust polluters of…

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marzo 2017

From the first stars to the first quasars

marzo 7 @ 11:45 - 12:45 - Oratore: Rosa Valiante (INAF - Osservatorio Astronomico di Roma)

Observations of the most luminous quasars at redshift z>6 reveal the existence of numerous supermassive…

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Highly Ionized X-ray Absorbers in AGNs and their Energetic: the case of NGC 4051

marzo 14 @ 11:45 - 12:45 - Oratore: Erendira Huerta Martinez (Osservatorio Astronomico di Roma)

Highly ionized absorbers are found in 50% of type 1 Seyferts and QSOs. They presence,…

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Dwarf Galaxies – Fossils of Galaxy Evolution

marzo 21 @ 11:45 - 12:45 - Oratore: Eva Grebel (Heidelberg)

Dwarf galaxies are the most common type of galaxy in the Universe and include the…

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The AGB-Supernovae mass transition

marzo 27 @ 9:00 - marzo 31 @ 18:00
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aprile 2017

The dust mass in Cassiopeia A from spatially resolved Herschel photometry

aprile 4 @ 11:45 - 12:45 - Oratore: Ilse De Looze (Gent University)

The large reservoirs of dust observed in some high redshift galaxies have been hypothesised to…

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Unveiling the most elusive star-forming galaxies

aprile 11 @ 11:45 - 12:45 - Oratore: Paola Santini (INAF - Osservatorio Astronomico di Roma)

Our knowledge of the cosmic star formation history is crucially dependent on completeness of the…

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Elemental Abundances across Cosmic Time

aprile 18 @ 11:45 - 12:45 - Oratore: Chiaki Kobayashi (University of Hertfordshire)

I show how chemical enrichment took place in the Milky Way and in a cosmic…

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The detection of magnetic waves in the solar atmosphere, using the Sun as plasma physics laboratory.

aprile 26 @ 11:45 - 12:45 - Oratore: Marco Stangalini (INAF - Osservatorio di Roma)

The Sun is one of our best plasma physics laboratory. The recent direct identification of…

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