Implications for accretion flow dynamics from a spectral study of Swift J1357.2–0933-Reference-Cited by-同舟云学术

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Implications for accretion flow dynamics from a spectral study of Swift J1357.2–0933

Published:2018-12-08 Issue:1 Volume:483 Page:1178-1183
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Mondal Santanu¹²,Chakrabarti Sandip K²³

Affiliation:

1. Instituto de Física y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, Gran Bretana N 1111, Playa Ancha, Valparaíso, Chile

2. Indian Centre for Space Physics, Chalantika 43, Garia Station Rd., Kolkata 700084, India

3. S. N. Bose National Centre for Basic Sciences, Kolkata 700098, India

Funder

Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica

California Institute of Technology

National Aeronautics and Space Administration

Goddard Space Flight Center

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/483/1/1178/27070326/sty3169.pdf

Reference61 articles.

1. Multiwavelength spectral evolution during the 2011 outburst of the very faint X-ray transient Swift J1357.2−0933

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

3. The Burst Alert Telescope (BAT) on the SWIFT Midex Mission

4. The 2004 outburst of BHC H1743-322: analysis of spectral and timing properties using the TCAF solution

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