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Modelling multiwavelength emissions from PSR B1259-63/LS 2883: Effects of the stellar disc on shock radiations

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成果类型:
期刊论文
作者:
Chen, A. M.*;Takata, J.;Yi, S. X.;Yu, Y. W.(俞云伟);Cheng, K. S.
通讯作者:
Chen, A. M.
作者机构:
[Yu, Y. W.; Chen, A. M.] Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Hubei, Peoples R China.
[Chen, A. M.; Yi, S. X.; Cheng, K. S.] Univ Hong Kong, Dept Phys, Pokfulam Rd, Hong Kong, Peoples R China.
[Takata, J.] Huazhong Univ Sci & Technol, Sch Phys, Wuhan 430074, Hubei, Peoples R China.
[Yi, S. X.] Radboud Univ Nijmegen, Dept Astrophys, POB 9010, NL-6500 GL Nijmegen, Netherlands.
通讯机构:
[Chen, A. M.] C
[Chen, A. M.] U
Cent China Normal Univ, Inst Astrophys, Wuhan 430079, Hubei, Peoples R China.
Univ Hong Kong, Dept Phys, Pokfulam Rd, Hong Kong, Peoples R China.
语种:
英文
关键词:
Binaries: close;Gamma rays: stars;Pulsars: individual: PSR B1259-63;X-rays: binaries
期刊:
ASTRONOMY AND ASTROPHYSICS
ISSN:
0004-6361
年:
2019
卷:
627
页码:
A87-
基金类别:
We are very grateful for the valuable suggestions and comments of the referee, which improved the manuscript significantly. J.T is supported by the National Science Foundation of China under 11573010, 11661161010, U1631103 and U1838102. Y.W.Y is supported by the National Natural Science Foundation of China under 11822302 and 11833003. K.S.C is supported by GRF grant under 17302315.
机构署名:
本校为第一且通讯机构
院系归属:
物理科学与技术学院
摘要:
PSR B1259-63/LS 2883 is an elliptical pulsar/Be star binary that emits broadband emissions from radio to TeV γ-rays. The massive star possesses an equatorial disc that is inclined with the orbital plane of the pulsar. Non-thermal emission from the system is believed to be produced by pulsar wind shock and double-peak profiles in the X-ray, and TeV γ-ray light curves are related to the phases of the pulsar passing through the disc region of the star. In this paper, we investigate the interactions between the pulsar wind and stellar outflows, e...

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