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Biases in the inferred mass-to-light ratio of globular clusters: no need for variations in the stellar mass function

Shanahan, RL and Gieles, M (2015) Biases in the inferred mass-to-light ratio of globular clusters: no need for variations in the stellar mass function MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 448 (1). L94-L98.

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Item Type: Article
Authors :
NameEmailORCID
Shanahan, RLUNSPECIFIEDUNSPECIFIED
Gieles, Mm.gieles@surrey.ac.ukUNSPECIFIED
Date : 21 March 2015
Identification Number : https://doi.org/10.1093/mnrasl/slu205
Uncontrolled Keywords : Science & Technology, Physical Sciences, Astronomy & Astrophysics, globular clusters: general, open clusters and associations: general, STAR-CLUSTERS, SIZE DIFFERENCE, BLACK-HOLES, GALAXIES, POPULATION, EVOLUTION, MODELS, RADII, RED, M3
Related URLs :
Depositing User : Symplectic Elements
Date Deposited : 17 May 2017 13:33
Last Modified : 17 May 2017 15:11
URI: http://epubs.surrey.ac.uk/id/eprint/839640

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