Evolution of high-mass X-ray binaries in the small magellanic cloud-Reference-Cited by-同舟云学术

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Evolution of high-mass X-ray binaries in the small magellanic cloud

Published:2019-01 Issue:1-3 Volume:340 Page:46-49
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron. Nachr.

Author:

Yang J.¹,Wik D. R.¹,Zezas A.²,Laycock S. G. T.³,Hong J.²,Xu R.⁴⁵

Affiliation:

1. Department of Physics and Astronomy; The University of Utah; Salt Lake City Utah

2. Harvard-Smithsonian Center for Astrophysics; Cambridge Massachusetts

3. Department of Physics and Applied Physics; University of Massachusetts; Lowell Massachusetts

4. School of Physics and State Key Laboratory of Nuclear Physics and Technology; Peking University; Beijing China

5. Kavli Institute for Astronomy and Astrophysics; Peking University; Beijing China

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/asna.201913557/fullpdf

Reference33 articles.

1. A new class of radio pulsars

2. A Radio Pulsar/X-ray Binary Link

3. Becker , W. Trümper , J 1997

4. Beskin , V. Balogh , A. Falanga , M. Lyutikov , M. Mereghetti , S. Piran , T. Treumann , R.

5. Formation and evolution of binary and millisecond radio pulsars

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