Is the escape velocity in star clusters linked to extended star formation histories? Using NGC 7252: W3 as a test case-Reference-Cited by-同舟云学术

Is the escape velocity in star clusters linked to extended star formation histories? Using NGC 7252: W3 as a test case

Published:2016-01-27 Issue:1 Volume:457 Page:809-821
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Cabrera-Ziri I.,Bastian N.,Hilker M.,Davies B.,Schweizer F.,Kruijssen J. M. D.,Mejía-Narváez A.,Niederhofer F.,Brandt T. D.,Rejkuba M.,Bruzual G.,Magris G.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/457/1/809/18168030/stv2977.pdf

Reference71 articles.

1. The Rotation Curve of the Large Magellanic Cloud and the Implications for Microlensing

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

3. The morphology of the sub-giant branch and red clump reveal no sign of age spreads in intermediate-age clusters

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

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