Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S329(12), p. 388-388, 2016
DOI: 10.1017/s1743921317001570
Links
Tools
Detectability of Wolf-Rayet stars in M33 and Beyond the Local Group
This paper was not found in any repository, but could be made available legally by the author.
Full text: Unavailable
Published version:
archiving forbidden
Data provided by 
Abstract
AbstractTo understand how complete our surveys of Wolf-Rayet (WR) stars can be with the current generation of telescopes, we study images of M33, a galaxy with a nearly complete WR catalogue, and degrade them to investigate the detectability of WRs out to 30Mpc. We lose almost half of our sample at 4.2Mpc, and at 30Mpc we detect only those WRs in bright regions.
