ИСТИНА

• Охват: Международная
• Даты проведения: 19-24 сентября 2016
• Место проведения: Париж, France
• Организатор:
  Institut d'Astrophysique de Paris
• Число участников: 120
• Число иностранных участников: 120
• Число участников из МГУ: 1
• Число докладчиков: 65
• Веб-сайт: http://www.iap.fr/vie_scientifique/ateliers/MilkyWay_Workshop/2016/
• Описание конференции:

  The level of detail we can attain through the study of individual stars, the interstellar medium, the birth places of stars, and the properties of dark matter in the Milky Way and its halo scale environment is such that we can begin to quantitatively constrain many of our ideas about the formation and evolution of our Galaxy and the Local Group. That is, we must view the Milky Way and its environment within the general context of galaxies and our theoretical and model understanding of how galaxies grow and evolve within the current cosmological framework. The more so, since our Galaxy appears to be a "typical" spiral in many ways: its total stellar mass is similar to that of the fiducial break mass in the galaxy mass function; during the peak of the star formation rate density, a large fraction of all stars formed in MW-progenitor massed galaxies; the structural components of the MW appear similar to other nearby spiral galaxies; the star formation history of the MW appears similar to galaxies of similar mass in the local universe; it's environmental density, number, and type of satellite galaxies appears pretty typical for its total stellar mass. In short, it appears that the MW can tell us a great deal about the evolutionary processes common to all galaxies

• Добавил в систему: Мельник Анна Маратовна

Доклады:

• 2016 Different models of the Galactic spiral structure: kinematical and morphological aspects (Устный)
• Автор: Мельник А.М.