State transitions of GRS 1739−278 in the 2014 outburst-Reference-Cited by-同舟云学术

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State transitions of GRS 1739−278 in the 2014 outburst

Published:2018-05-25 Issue:4 Volume:70 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Wang Sili¹,Kawai Nobuyuki¹,Shidatsu Megumi²,Tachibana Yutaro¹,Yoshii Taketoshi¹,Sudo Masayuki³,Kubota Aya³

Affiliation:

1. Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro, Tokyo 152-8551, Japan

2. MAXI team, Institute of Physical and Chemical Research (RIKEN), Wako, 2-1 Hirosawa, Saitama 351-0198, Japan

3. Department of Electrical and Information Systems, Shibuya Institute of Technology, 307 Fukasaku, Minuma, Saitama City, Saitama 337-8570, Japan

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/70/4/67/25439085/psy058.pdf

Reference41 articles.

1. Detection of a 5 H[CLC]z[/CLC] Quasi-periodic Oscillation from X-Ray Nova GRS 1739−278

2. The Swift X-Ray Telescope

3. Anti-correlated hard and soft X-ray intensity variations of the black-hole candidates Cyg X-1 and A0620—00

4. BlackCAT: A catalogue of stellar-mass black holes in X-ray transients

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