Rapid orbital expansion in millisecond pulsar PSR J0636+5128: evaporation winds?
Author:
Affiliation:
1. School of Science, Qingdao University of Technology, Qingdao 266525, China
2. School of Physics and Electrical Information, Shangqiu Normal University, Shangqiu 476000, China
Abstract
Funder
National Natural Science Foundation of China
Henan University
China Scholarship Council
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staa3701/34571787/staa3701.pdf
Reference63 articles.
1. A new class of radio pulsars
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3. A Radio Pulsar/X-ray Binary Link
4. The NANOGrav 11-year Data Set: High-precision Timing of 45 Millisecond Pulsars
5. Transformation of a Star into a Planet in a Millisecond Pulsar Binary
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2. Binding energy produced within the framework of the accretion of millisecond pulsars;Chinese Physics C;2023-04-01
3. On the effect of pulsar evaporation on the cooling of white dwarfs;MON NOT R ASTRON SOC;2021
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