The high mass end of the stellar mass function: Dependence on stellar population models and agreement between fits to the light profile (2017)
Attributed to:
Astrophysics at Southampton
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stx176
Publication URI: http://dx.doi.org/10.1093/mnras/stx176
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society