The minimum magnetic field of millisecond pulsars calculated according to accretion: application to the X-ray neutron star SAX J1808.4–3658 in a low-mass X-ray binary-Reference-Cited by-同舟云学术

The minimum magnetic field of millisecond pulsars calculated according to accretion: application to the X-ray neutron star SAX J1808.4–3658 in a low-mass X-ray binary

Published:2018-07-28 Issue:1 Volume:480 Page:692-696
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Pan Y Y¹²,Zhang C M²³⁴,Song L M⁵,Wang N⁶,Li D²³^ORCID,Yang Y Y²³⁷

Affiliation:

1. Department of Physics, Xiangtan University, Hunan 411105, China

2. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China

3. CAS Key Laboratory of FAST, Chinese Academy of Sciences, Beijing 100101, China

4. School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 101400, China

5. Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

6. Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, China

7. Astronomy Department, Beijing Normal University, Beijing 100875, China

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/480/1/692/25262047/sty1851.pdf

Reference63 articles.

1. A new class of radio pulsars

2. A millisecond pulsar

3. Formation and evolution of binary and millisecond radio pulsars

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