Orbital evolution and search for eccentricity and apsidal motion in the eclipsing HMXB 4U 1700−37
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/461/1/816/8042903/stw1299.pdf
Reference55 articles.
1. Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors
2. The origin of the runaway high-mass X-ray binary HD 153919/4U1700-37
3. A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
4. Further Copernicus X-ray observations of 3U 1700-37.
5. Wind-driven angular momentum loss in binary systems. I - Ballistic case
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