APIE TFAISeminaro vadovas - habil. dr. Antanas BARTKEVIČIUS
Seminaro vadovo pavaduotojas - dr. Julius SPERAUSKAS
Seminaro sekretorė - dr. Erika PAKŠTIENĖ
Tematika: astronomija
Periodiškumas: antradieniais 14 val. Vilniuje Goštauto 12, 432 k.
Pranešėjų ir klausytojų kontingentas: Vilniaus astronomai ir astronomijos doktorantai, retkarčiais užsienio astronomai.
Detalesnė informacija:
tel. 2613440, el. paštas: bart@itpa.lt,
tel. 2398763, el. paštas julius.sperauskas@ff.vu.lt
Mark Gieles (Institute of Astronomy, Cambridge) pranešimas "Young Massive Clusters"
Kviečiame į Vilniaus universiteto astronominių seminarų ciklo
"Šiuolaikinės astrofizikos problemos" šeštąją dalį, kuri įvyks
2011 m. lapkričio 16 d. (trečiadienį) 14 val. VU TFAI (A. Goštauto g.
12) ketvirtojo aukšto salėje.
Mark Gieles (Institute of Astronomy, Cambridge)
Young Massive Clusters
Young massive clusters (YMCs) are dense aggregates of young stars. Several examples exist in the Milky Way Galaxy and the Local Group, but they are particularly abundant in starburst and interacting galaxies. The few YMCs that are close enough to resolve are of prime interest for studying the stellar mass function and the ecological interplay between stellar evolution and stellar dynamics. The distant unresolved clusters may be effectively used to study the star-cluster mass function, and they provide constraints on the formation mechanisms of young cluster populations. We describe the global properties of the currently known young massive star clusters in the Local Group and beyond, and discuss the state of the art in observations and dynamical modeling of these systems.
Maloniai kviečiame dalyvauti!
Seminarų ciklo organizatoriai,
Arūnas Kučinskas
Donatas Narbutis
Mark Gieles (Institute of Astronomy, Cambridge)
Young Massive Clusters
Young massive clusters (YMCs) are dense aggregates of young stars. Several examples exist in the Milky Way Galaxy and the Local Group, but they are particularly abundant in starburst and interacting galaxies. The few YMCs that are close enough to resolve are of prime interest for studying the stellar mass function and the ecological interplay between stellar evolution and stellar dynamics. The distant unresolved clusters may be effectively used to study the star-cluster mass function, and they provide constraints on the formation mechanisms of young cluster populations. We describe the global properties of the currently known young massive star clusters in the Local Group and beyond, and discuss the state of the art in observations and dynamical modeling of these systems.
Maloniai kviečiame dalyvauti!
Seminarų ciklo organizatoriai,
Arūnas Kučinskas
Donatas Narbutis
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