The Orbital Period of SMC X-3 from Optical Photometry
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference22 articles.
1. Calibration of the MACHO Photometry Database
2. Extreme variability in the Be-type, periodic recurrent X-ray transient A0538 - 66: a highly eccentric interacting binary
3. On two new X-ray sources in the SMC and the high luminosities of the Magellanic X-ray sources
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1. Population Synthesis of Ultraluminous X-ray Sources with Magnetized Neutron Stars;Astronomy Letters;2020-10
2. Accreting, highly magnetized neutron stars at the Eddington limit: a study of the 2016 outburst of SMC X-3;Astronomy & Astrophysics;2018-06
3. SMC X-3: the closest ultraluminous X-ray source powered by a neutron star with non-dipole magnetic field;Astronomy & Astrophysics;2017-09
4. The 2016 super-Eddington outburst of SMC X-3: X-ray and optical properties and system parameters;Monthly Notices of the Royal Astronomical Society;2017-07-25
5. SwiftObservations of SMC X-3 during Its 2016–2017 Super-Eddington Outburst;The Astrophysical Journal;2017-07-05
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