|
Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://lnfm1.sai.msu.ru/~zabolot/announce.htm
Дата изменения: Tue Mar 29 10:20:22 2016 Дата индексирования: Sun Apr 10 00:25:00 2016 Кодировка: Windows-1251 Поисковые слова: п п р п р п р п |
6 апреля (СРЕДА) в 13 часов 00 минут в 48 аудитории ГАИШ МГУ состоится Семинар по звездной астрономии
Повестка дня:Anil Pandey (ARIES, Manora Peak, Nainital 263002, India)
"Triggered Star Formation"
It is now well established that massive stars in star forming regions can trigger next generation of star formation. Theoretical simulations suggest two main processes for triggered star formation; the radiation driven implosion (RDI) process and collect & collapse (CC) process. In this talk I will discuss observational aspects of triggered star formation scenario. The young stellar objects (YSOs) in star forming regions have been identified using the near-infrared (NIR) and mid-infrared (MIR) observations. The age of the identified YSOs was estimated using the optical color-magnitude diagram. The age of YSOs, the morphology of the regions and the global distribution of YSOs indicate that the star formation can be triggered by either (RDI/ CC) of the processes.
40 мин.