Comparison of spectral models for disc truncation in the hard state of GX 339–4-Reference-Cited by-同舟云学术

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Comparison of spectral models for disc truncation in the hard state of GX 339–4

Published:2019-03-08 Issue:3 Volume:485 Page:3845-3856
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Dziełak Marta A¹,Zdziarski Andrzej A¹,Szanecki Michał¹,De Marco Barbara¹,Niedźwiecki Andrzej²,Markowitz Alex¹³

Affiliation:

1. Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, PL-00-716 Warszawa, Poland

2. Department of Astrophysics, Łódź University, Pomorska 149/153, PL-90-236 Łódź, Poland

3. Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Dr, La Jolla, CA 92093-0424, USA

Funder

Polish National Science Centre

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/485/3/3845/28230411/stz668.pdf

Reference84 articles.

1. A Bayesian analysis of the minimum AIC procedure

2. Abundances of the elements: Meteoritic and solar

3. Breaking the spectral degeneracies in black hole binaries with fast timing data: the hard state of Cygnus X-1

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3. High-density Reflection Spectroscopy of Black Hole X-Ray Binaries in the Hard State;The Astrophysical Journal;2023-07-01

4. The Hard-to-soft Transition of GX 339–4 as Seen by Insight–HXMT;The Astrophysical Journal;2023-06-01

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