Optical studies of two Large Magellanic Cloud X-ray transients: RX J0544.1-7100 and RX J0520.5-6932-Reference-Cited by-同舟云学术

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Optical studies of two Large Magellanic Cloud X-ray transients: RX J0544.1-7100 and RX J0520.5-6932

Published:2001-06-21 Issue:3 Volume:324 Page:623-627
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Coe M. J.,Negueruela I.,Buckley D. A. H.,Haigh N. J.,Laycock S. G. T.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/324/3/623/3384360/324-3-623.pdf

Reference14 articles.

1. A 421-d activity cycle in the BeX recurrent transient A0538-66 from MACHO monitoring

2. Extreme variability in the Be-type, periodic recurrent X-ray transient A0538 - 66: a highly eccentric interacting binary

3. Rossi X‐Ray Timing ExplorerObservations of the X‐Ray Pulsar XTE J1855−026: A Possible New Supergiant System

4. Four outburst cycles of A 0538 - 66: evidence for a rapidly evolving envelope around the primary

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2. The Ups and Downs of Accreting X-Ray Pulsars: Decade-long Observations with the Fermi Gamma-Ray Burst Monitor;The Astrophysical Journal;2020-06-16

3. Correlation between the luminosity and spin-period changes during outbursts of 12 Be binary pulsars observed by the MAXI/GSC and the Fermi/GBM;Publications of the Astronomical Society of Japan;2017-12-01

4. Transient X-Ray Sources in the Magellanic-type Galaxy NGC 4449;The Astrophysical Journal;2017-02-07

5. TRACING THE LOWEST PROPELLER LINE IN MAGELLANIC HIGH-MASS X-RAY BINARIES;The Astrophysical Journal;2016-09-20

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