The young star cluster population of M51 with LEGUS: II. testing environmental dependences

Abstract. It has recently been established that the properties of young star clusters (YSCs) can vary as a function of the galactic environment in which they a

Saved in:

Bibliographic Details
Main Authors:	Messa, Matteo (Author) , Reina-Campos, Marta (Author) , Gouliermis, Dimitrios A. (Author) , Grebel, Eva K. (Author) , Kruijssen, Diederik (Author)
Format:	Article (Journal)
Language:	English
Published:	2018 March 23
In:	Monthly notices of the Royal Astronomical Society Year: 2018, Volume: 477, Issue: 2, Pages: 1683-1707
ISSN:	1365-2966
DOI:	10.1093/mnras/sty577
Online Access:	Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty577 Verlag, Volltext: https://academic.oup.com/mnras/article/477/2/1683/4952003
Author Notes:	Matteo Messa, A. Adamo, D. Calzetti, M. Reina-Campos, D. Colombo, E. Schinnerer, R. Chandar, D.A. Dale, D.A. Gouliermis, K. Grasha, E.K. Grebel, B.G. Elmegreen, M. Fumagalli, K.E. Johnson, J.M.D. Kruijssen, G. Östlin, F. Shabani, L.J. Smith and B.C. Whitmore

Description
Summary:	Abstract. It has recently been established that the properties of young star clusters (YSCs) can vary as a function of the galactic environment in which they a
Item Description:	Gesehen am 06.02.2019
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/sty577