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DTSTART;TZID=Europe/Rome:20160517T114500
DTEND;TZID=Europe/Rome:20160517T124500
DTSTAMP:20260405T012638
CREATED:20160405T045745Z
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UID:1048-1463485500-1463489100@www.oa-roma.inaf.it
SUMMARY:Evolution of close binary systems
DESCRIPTION:A general outlook of the evolution of close binary stars and of population synthesis as a method of their study will be presented. I will pay special attention to the evolution of low- and intermediate-mass stars (M < (8-10) solar) and to formation of different still hypothetical progenitors of SNe Ia. Next\, I will consider evolution of massive binaries with an accent on scenarii of evolution leading to the recently discovered gravitational waves burst GW150914
URL:https://www.oa-roma.inaf.it/event/evolution-of-close-binary-systems/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20160517T114500
DTEND;TZID=Europe/Rome:20160517T124500
DTSTAMP:20260405T012638
CREATED:20160405T045745Z
LAST-MODIFIED:20160405T045745Z
UID:4665-1463485500-1463489100@www.oa-roma.inaf.it
SUMMARY:Evolution of close binary systems
DESCRIPTION:A general outlook of the evolution of close binary stars and of population synthesis as a method of their study will be presented. I will pay special attention to the evolution of low- and intermediate-mass stars (M < (8-10) solar) and to formation of different still hypothetical progenitors of SNe Ia. Next\, I will consider evolution of massive binaries with an accent on scenarii of evolution leading to the recently discovered gravitational waves burst GW150914
URL:https://www.oa-roma.inaf.it/event/evolution-of-close-binary-systems-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
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