The advection-dominated accretion flow for the origin of the thermal soft X-ray component in low-level accreting neutron stars-Reference-Cited by-同舟云学术

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The advection-dominated accretion flow for the origin of the thermal soft X-ray component in low-level accreting neutron stars

Published:2018-08-25 Issue:1 Volume:481 Page:938-946
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Qiao Erlin¹²,Liu B F¹²

Affiliation:

1. Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China

2. School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, 19A Yuquan Road, Beijing 100049, China

Funder

National Natural Science Foundation of China

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/481/1/938/25697722/sty2337.pdf

Reference62 articles.

1. Thermal equilibria of accretion disks

2. The X-ray spectral properties of very-faint persistent neutron star X-ray binaries

3. XMM–Newton and Swift spectroscopy of the newly discovered very faint X-ray transient IGR J17494–3030

4. XMM–Newton and Swift spectroscopy of the newly discovered very faint X-ray transient IGR J17494–3030

5. DISCOVERY OF THE THIRD TRANSIENT X-RAY BINARY IN THE GALACTIC GLOBULAR CLUSTER TERZAN 5

Cited by 7 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. Simultaneous Chandra and HST observations of the quiescent neutron star low-mass X-ray binaries in 47 Tucanae;Monthly Notices of the Royal Astronomical Society;2024-04-27

2. The radiative efficiency of neutron stars at low-level accretion;Monthly Notices of the Royal Astronomical Society;2021-01-28

3. The advection-dominated accretion flow for the anticorrelation between the X-ray photon index and the X-ray luminosity in neutron star low-mass X-ray binaries;Monthly Notices of the Royal Astronomical Society;2020-06-12

4. Two-temperature Radiative Hot Accretion Flow around Neutron Stars;The Astrophysical Journal;2020-02-19

5. A systematic study of the advection-dominated accretion flow for the origin of the X-ray emission in weakly magnetized low-level accreting neutron stars;Monthly Notices of the Royal Astronomical Society;2019-12-16

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