Constraints on the number of X-ray pulsars in IC 10 from a deep XMM-Newton observation
Author:
Affiliation:
1. Department of Physics and Astronomy; The University of Utah; Salt Lake City Utah
2. Department of Physics and Applied Physics; University of Massachusetts; Lowell Massachusetts
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1002/asna.201913561/fullpdf
Reference50 articles.
1. ASTROPHYSICAL IMPLICATIONS OF THE BINARY BLACK HOLE MERGER GW150914
2. Star formation history and X-ray binary populations: the case of the Large Magellanic Cloud
3. STAR FORMATION HISTORY AND X-RAY BINARY POPULATIONS: THE CASE OF THE SMALL MAGELLANIC CLOUD
4. NGC 300 X-1 and IC 10 X-1: a new breed of black hole binary?
5. Discovery of pulsations from NGC 300 ULX1 and its fast period evolution
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