Stellar Populations in the Magellanic Clouds

التفاصيل البيبلوغرافية
العنوان:	Stellar Populations in the Magellanic Clouds
المؤلفون:	Feast, M.W.
المصدر:	Symposium - International Astronomical Union ; volume 164, page 153-163 ; ISSN 0074-1809
بيانات النشر:	Cambridge University Press (CUP)
سنة النشر:	1995
الوصف:	There seems to be no strong evidence that the young globular clusters in the MC have metallicities differing significantly from the metallicities of MC field stars of the same age. The old globular clusters in the LMC are of the same age as, or slightly younger than, those in the outer halo of our Galaxy. It is suggested that the increase in the SFR in the LMC ~ 4 Gyr ago was related to the collapse of the system to a plane. Evidence for a spread in metallicities amongst young stars in either Cloud remains tentative. There is no strong evidence for bursts of star formation being triggered by LMC-SMC-Galaxy interactions but the possibility is raised that the SFR in the SMC has been strongly affected by this interaction.
نوع الوثيقة:	article in journal/newspaper
اللغة:	English
DOI:	10.1017/s0074180900108526
الاتاحة:	http://dx.doi.org/10.1017/s0074180900108526 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S0074180900108526
Rights:	https://www.cambridge.org/core/terms
رقم الانضمام:	edsbas.D8B1B380
قاعدة البيانات:	BASE

الوصف
DOI:	10.1017/s0074180900108526