Accretion geometry of the black-hole binary Cygnus X-1 from X-ray polarimetry-Reference-Cited by-同舟云学术

Accretion geometry of the black-hole binary Cygnus X-1 from X-ray polarimetry

Published:2018-06-25 Issue:8 Volume:2 Page:652-655
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Chauvin M.,Florén H.-G.,Friis M.,Jackson M.,Kamae T.,Kataoka J.,Kawano T.,Kiss M.^ORCID,Mikhalev V.^ORCID,Mizuno T.,Ohashi N.,Stana T.,Tajima H.,Takahashi H.^ORCID,Uchida N.,Pearce M.^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-018-0489-x.pdf

Reference41 articles.

1. Remillard, R. A. & McClintock, J. E. X-ray properties of black-hole binaries. Annu. Rev. Astron. Astr. 44, 49–92 (2006).

2. Makishima, K. et al. Suzaku results on Cygnus X-1 in the low/hard state. Publ. Astron. Soc. Jpn 60, 585–604 (2008).

3. Fabian, A. C. et al. On the determination of the spin of the black hole in Cyg X-1 from X-ray reflection spectra. Mon. Not. R. Astron. Soc. 424, 217–223 (2012).

4. Webster, B. L. & Murdin, P. Cygnus X-1-a spectroscopic binary with a heavy companion? Nature 235, 37–28 (1972).

5. Miniutti, G. & Fabian, A. C. A light bending model for the X-ray temporal and spectral properties of accreting black holes. Mon. Not. R. Astron. Soc. 349, 1435–1448 (2004).

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