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

Cabrera-Ziri, I., Bastian, N., Hilker, M., Davies, B., Schweizer, F., Kruijssen, J. M. D., et al. (2016). Is the escape velocity in star clusters linked to extended star formation histories? Using NGC 7252: W3 as a test case. Monthly Notices of the Royal Astronomical Society, 457(1), 809-821. doi:10.1093/mnras/stv2977.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-002A-38E9-0 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-002A-38EA-E
Genre: Journal Article

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 Creators:
Cabrera-Ziri, I., Author
Bastian, N., Author
Hilker, M., Author
Davies, B., Author
Schweizer, F., Author
Kruijssen, J. M. D.1, Author           
Mejía-Narváez, A., Author
Niederhofer, F., Author
Brandt, T. D., Author
Rejkuba, M., Author
Bruzual, G., Author
Magris, G., Author
Affiliations:
1Computational Structure Formation, MPI for Astrophysics, Max Planck Society, ou_2205642              

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Language(s): eng - English
 Dates: 2016-03-21
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1093/mnras/stv2977
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Title: Monthly Notices of the Royal Astronomical Society
  Abbreviation : Mon. Not. R. Astr. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 457 (1) Sequence Number: - Start / End Page: 809 - 821 Identifier: ISSN: 0035-8711