Orbital period variations in eclipsing post-common-envelope binaries-Reference-Cited by-同舟云学术

Orbital period variations in eclipsing post-common-envelope binaries

Published:2010-07-20 Issue:4 Volume:407 Page:2362-2382
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Parsons S. G.,Marsh T. R.,Copperwheat C. M.,Dhillon V. S.,Littlefair S. P.,Hickman R. D. G.,Maxted P. F. L.,Gänsicke B. T.,Unda-Sanzana E.,Colque J. P.,Barraza N.,Sánchez N.,Monard L. A. G.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/407/4/2362/17325969/mnras0407-2362.pdf

Reference47 articles.

1. Cataclysmic Variables: An Empirical Angular Momentum Loss Prescription from Open Cluster Data

2. A mechanism for orbital period modulation in close binaries

3. Detection of a period decrease in NN Ser with ULTRACAM: evidence for strong magnetic braking or an unseen companion

4. The Eclipsing Precataclysmic Binary RR Caeli

5. Physical properties of IP Pegasi: an eclipsing dwarf nova with an unusually cool white dwarf

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