A New Orbital Ephemeris and Reinterpretation of Spectroscopic Data for the Supersoft X-Ray Binary RX J0513.9−6951
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference14 articles.
1. Calibration of the MACHO Photometry Database
2. Cowley, A. P., Schmidtke, P. C., Crampton, D. & Hutchings, J. B. 1996, in IAU Symp. 165, Compact Stars in Binaries, ed. J. van Paradijs, E. P. J. van den Heuvel, & E. Kuulkers (Dordrecht: Kluwer), 439
3. Six Supersoft X‐Ray Binaries: System Parameters and Twin‐Jet Outflows
4. Detection, Identification, and Observed Properties of Large Magellanic Cloud Supersoft X-Ray Sources
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1. A robust model for the origin of optical quasi-periodic variability in supersoft X-ray sources;Astronomy & Astrophysics;2022-10
2. Multiwavelength Modeling the SED of Luminous Supersoft X-Ray Sources in Large Magellanic Cloud and Small Magellanic Cloud;The Astronomical Journal;2022-09-19
3. Optical and X-ray properties of CAL 83 – I. Quasi-periodic optical and supersoft variability;Monthly Notices of the Royal Astronomical Society;2013-05-10
4. Supersoft X-ray sources: Confronting the van den Heuvel paradigm;New Astronomy Reviews;2010-03
5. Variability in the cycle length of the supersoft source RX J0513.9-6951;Astronomy & Astrophysics;2008-02-04
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