Discovery of a 26.2 day period in the long-term X-ray light curve of SXP 1323: a very short orbital period for a long spin period pulsar
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201629299/pdf
Reference35 articles.
1. On the periodicities present in the optical light curves of Small Magellanic Cloud Be/X-ray binaries
2. Catalogue of Be/X-ray binary systems in the Small Magellanic Cloud: X-ray, optical and IR properties
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4. The XMM-Newton survey of the Small Magellanic Cloud: XMMU J005011.2−730026 = SXP 214, a Be/X-ray binary pulsar★
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1. Discovery of a Rare Eclipsing Be/X-Ray Binary System, Swift J010902.6-723710 = SXP 182;The Astrophysical Journal Letters;2024-04-01
2. Spectral and timing properties of the recently discovered Be/X-ray pulsar eRASSUJ 052914.9−662446;Monthly Notices of the Royal Astronomical Society;2022-09-30
3. Losing a minute every two years: SRG X-ray view of the rapidly accelerating X-ray pulsar SXP 1323;Astronomy & Astrophysics;2021-12-05
4. SRG/eROSITA discovery of 164s pulsations from the SMC Be/X-ray binary XMMU J010429.4-723136;Astronomy & Astrophysics;2021-11-01
5. Population Synthesis of Neutron Star X-Ray Binaries Associated with Supernova Remnants;The Astrophysical Journal;2021-10-01
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