Radio pulsations from a neutron star within the gamma-ray binary LS I +61° 303-Reference-Cited by-同舟云学术

Radio pulsations from a neutron star within the gamma-ray binary LS I +61° 303

Published:2022-03-17 Issue:6 Volume:6 Page:698-702
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Weng Shan-Shan^ORCID,Qian Lei^ORCID,Wang Bo-Jun,Torres D. F.^ORCID,Papitto A.,Jiang Peng,Xu Renxin,Li Jian^ORCID,Yan Jing-Zhi,Liu Qing-Zhong,Ge Ming-Yu,Yuan Qi-Rong

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-022-01630-1.pdf

Reference52 articles.

1. Dubus, G. Gamma-ray binaries and related systems. Astron. Astrophys. Rev. 21, 64 (2013).

2. Abdo, A. A., Ackermann, M. & Ajello, M. et al. Fermi LAT observations of LS I +61 303: first detection of an orbital modulation in GeV gamma rays. Astrophys. J. Lett. 701, L123–L128 (2009).

3. Gregory, P. C. Bayesian analysis of radio observations of the Be X-ray binary LS I +61 303. Astrophys. J. 575, 427–434 (2002).

4. Albert, J., Aliu, E. & Anderhub, H. et al. Multiwavelength (radio, X-ray, and γ-ray) observations of the γ-ray binary LS I +61 303. Astrophys. J. 684, 1351–1358 (2008).

5. Dhawan, V., Mioduszewski, A. & Rupen, M. LS I +61 303 is a Be-pulsar binary, not a microquasar. In VI Microquasar Workshop: Microquasars and Beyond 52.1 (ed. Belloni, T.) (Proceedings of Science, 2006).

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