Discovery of the 10.6 hr orbital period of CAL87: an eclipsing low-mass X-ray binary in the Large Magellanic Cloud-Reference-Cited by-同舟云学术

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Discovery of the 10.6 hr orbital period of CAL87: an eclipsing low-mass X-ray binary in the Large Magellanic Cloud

Published:1989-11-01 Issue:1 Volume:241 Page:37P-41P
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:

Callanan P. J.,Machin G.,Naylor T.,Charles P. A.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/241/1/37P/3188052/mnras241-037P.pdf

Cited by 24 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Spectral Modeling of the Supersoft X-Ray Source CAL87 Based on Radiative Transfer Codes;The Astrophysical Journal;2023-12-21

2. Revised ephemeris and orbital period derivative of the supersoft X-ray source CAL 87 based on 34 yr of observations;Monthly Notices of the Royal Astronomical Society;2023-11-27

3. THE X-RAY ECLIPSE GEOMETRY OF THE SUPER-SOFT X-RAY SOURCE CAL 87;The Astrophysical Journal;2014-08-11

4. WIND-DRIVEN EVOLUTION OF WHITE DWARF BINARIES TO TYPE Ia SUPERNOVAE;The Astrophysical Journal;2013-12-13

5. The outburst of Nova CSS 081007:030559+054715 (HV Ceti);Astronomy & Astrophysics;2012-09

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