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Evolution of accretion disc geometry of GRS 1915+105 during its χ state as revealed by TCAF solution

  • Published:2018-06-14 Issue:2 Volume:479 Page:2183-2192
  • ISSN:0035-8711
  • Container-title:Monthly Notices of the Royal Astronomical Society
  • language:en
  • Short-container-title:

Author:

Dutta Broja G12,Pal Partha Sarathi3,Chakrabarti Sandip K24

Affiliation:

1. Department of Physics, Rishi Bankim Chandra College, Naihati, W.B. 743165, India

2. Indian Centre for Space Physics, Kolkata 700084, India

3. Sun Yat-sen University, 135 West Xingang Road, Guangzhou 510275, China

4. S. N. Bose National Centre For Basic Sciences, Kolkata 700098, India

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 8 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. First detection of soft-lag in GRS 1915 + 105 at HFQPO using AstroSat observations;Monthly Notices of the Royal Astronomical Society;2023-11-09

2. Long-term X-ray observations of seyfert 1 galaxy ark 120: on the origin of soft-excess;Monthly Notices of the Royal Astronomical Society;2021-06-14

3. A variable corona for GRS 1915+105;Monthly Notices of the Royal Astronomical Society;2021-03-22

4. Time-domain variability properties of XTE J1650−500 during its 2001 outburst: evidence of disc–jet connection;Monthly Notices of the Royal Astronomical Society;2020-08-06

5. On the properties of dissipative shocks in the relativistic accretion flows;Monthly Notices of the Royal Astronomical Society;2020-07-13
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