Long-term periodicity in LS I +61°303 as beat frequency between orbital and precessional rate-Reference-Cited by-同舟云学术

Long-term periodicity in LS I +61°303 as beat frequency between orbital and precessional rate

Published:2013-06 Issue: Volume:554 Page:A105
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Massi M.,Jaron F.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201219685/pdf

Reference46 articles.

1. Multiwavelength (Radio, X‐Ray, and γ‐Ray) Observations of the γ‐Ray Binary LS I +61 303

2. On the Mechanism of Accretion by Stars

3. The radio to TeV orbital variability of the microquasar LS I +61 303

4. Cornwell, T., & Fomalont, E. B. 1999, in Synthesis Imaging in Radio Astronomy II, eds. G. B. Taylor, C. L. Carilli, & R. A. Perley, ASP Conf. Ser., 180, 187

5. Dhawan, V., Mioduszewski, A., & Rupen, M. 2006, in Proc. VI Microquasar Workshop, 52.1

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3. Energy-dependent periodicities of LS I +61°303 in the GeV band;Monthly Notices of the Royal Astronomical Society;2023-08-07

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