The shape of the initial cluster mass function: What it tells us about the local star formation efficiency

Parmentier, G., Goodwin, S.P., Kroupa, P. et al. (1 more author) (2008) The shape of the initial cluster mass function: What it tells us about the local star formation efficiency. Astrophysical Journal, 678. pp. 347-352. ISSN 0004-637X

Abstract

Metadata

Authors/Creators:
  • Parmentier, G.
  • Goodwin, S.P.
  • Kroupa, P.
  • Baumgardt, H.
Copyright, Publisher and Additional Information: © 2008 American Astronomical Society. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: galaxies : star clusters; stars : formation; stellar dynamics
Dates:
  • Published: 1 May 2008
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Depositing User: Symplectic Sheffield
Date Deposited: 16 Feb 2018 12:58
Last Modified: 16 Feb 2018 12:58
Published Version: https://doi.org/10.1086/587137
Status: Published
Publisher: American Astronomical Society
Refereed: Yes
Identification Number: https://doi.org/10.1086/587137

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