Superhump period of the black hole X-ray binary GX 339−4-Reference-Cited by-同舟云学术

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Superhump period of the black hole X-ray binary GX 339−4

Published:2018-06-27 Issue:4 Volume:478 Page:4710-4719
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Kosenkov Ilia A¹²^ORCID,Veledina Alexandra¹³⁴^ORCID

Affiliation:

1. Department of Physics and Astronomy, FI-20014 University of Turku, Finland

2. Department of Astrophysics, St Petersburg State University, Universitetskiy Pr. 28, Peterhof, 198504 St Petersburg, Russia

3. Nordita, KTH Royal Institute of Technology and Stockholm University, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden

4. Space Research Institute of the Russian Academy of Sciences, Profsoyuznaya Str. 84/32, Moscow 117997, Russia

Funder

Academy of Finland

Ministry of Education and Science of the Russian Federation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/478/4/4710/25100738/sty1142.pdf

Reference39 articles.

1. The 2002 Outburst of the Black Hole X‐Ray Binary 4U 1543−47: Optical and Infrared Light Curves

2. OPTICAL AND NEAR-INFRARED MONITORING OF THE BLACK HOLE X-RAY BINARY GX 339-4 DURING 2002-2010

3. Overview of an extensive multi-wavelength study of GX 339−4 during the 2010 outburst

4. Observations of the X-ray Nova GRO J0422+32. 1: Outburst and the decay to quiescence

5. Mass Measurements of Stellar and Intermediate-Mass Black Holes

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2. High-precision broadband linear polarimetry of early-type binaries;Astronomy & Astrophysics;2023-09

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4. The prototype X-ray binary GX 339–4: using TeV γ-rays to assess LMXBs as Galactic cosmic ray accelerators;Monthly Notices of the Royal Astronomical Society;2022-01-10

5. HFQPOs and discoseismic mode excitation in eccentric, relativistic discs. I. Hydrodynamic simulations;Monthly Notices of the Royal Astronomical Society;2020-07-08

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