Constraining globular cluster formation through studies of young massive clusters – III. A lack of gas and dust in massive stellar clusters in the LMC and SMC-Reference-Cited by-同舟云学术

Constraining globular cluster formation through studies of young massive clusters – III. A lack of gas and dust in massive stellar clusters in the LMC and SMC

Published:2014-08-09 Issue:4 Volume:443 Page:3594-3600
ISSN:1365-2966
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Bastian N.,Strader J.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/443/4/3594/6295169/stu1407.pdf

Reference45 articles.

1. The effect of stellar rotation on colour-magnitude diagrams: on the apparent presence of multiple populations in intermediate age stellar clusters

2. Constraints on possible age spreads within young massive clusters in the Large Magellanic Cloud

3. Early disc accretion as the origin of abundance anomalies in globular clusters

4. Constraining globular cluster formation through studies of young massive clusters – I. A lack of ongoing star formation within young clusters

5. Testing stellar population models with star clusters in the Large Magellanic Cloud

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