OGLE observations of four X-ray binary pulsars in the Small Magellanic Cloud
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/311/1/169/3137147/311-1-169.pdf
Reference17 articles.
1. Ellipsoidal light variations and masses of X-ray binaries
2. On two new X-ray sources in the SMC and the high luminosities of the Magellanic X-ray sources
3. The identification of the optical/IR counterpart to the ROSAT SMC X-ray transient RX J0117.6--7330
4. Approximations to the radii of Roche lobes
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2. High-mass X-ray binaries in the Small Magellanic Cloud;Astronomy & Astrophysics;2016-01-28
3. An analysis of optical periods in individual Small Magellanic Cloud Be/X-ray pulsars;Monthly Notices of the Royal Astronomical Society;2013-02-27
4. THECHANDRASURVEY OF THE SMALL MAGELLANIC CLOUD “BAR”. II. OPTICAL COUNTERPARTS OF X-RAY SOURCES;The Astrophysical Journal;2009-05-14
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