Understanding X-ray irradiation in low-mass X-ray binaries directly from their light-curves-Reference-Cited by-同舟云学术

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Understanding X-ray irradiation in low-mass X-ray binaries directly from their light-curves

Published:2018-07-06 Issue:1 Volume:480 Page:2-16
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Tetarenko BE¹,Dubus G²,Lasota J-P³⁴,Heinke CO¹,Sivakoff GR¹

Affiliation:

1. Department of Physics, University of Alberta, CCIS 4-181, Edmonton, AB T6G 2E1, Canada

2. Institut de Planétologie et d’Astrophysique de Grenoble (IPAG), Univ. Grenoble Alpes, CNRS, F-38000, Grenoble, France

3. Institut d’Astrophysique de Paris, CNRS et Sorbonne Université, UMR 7095, 98bis Bd Arago, F-75014 Paris, France

4. Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, PL-00-716 Warsaw, Poland

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/480/1/2/25231090/sty1798.pdf

Reference67 articles.

1. An X-ray view of the very faint black hole X-ray transient Swift J1357.2–0933 during its 2011 outburst

2. Spectral analysis of theXMM–Newtondata of GX 339–4 in the low/hard state: disc truncation and reflection

3. The nature of dwarf nova outbursts

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