Orbital Period Increase in ES Ceti
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/852/i=1/a=19/pdf
Reference38 articles.
1. A mechanism for orbital period modulation in close binaries
2. Total eclipse of the heart: the AM CVn Gaia14aae/ASSASN-14cn
3. The photometric period in ES Ceti
4. Accretion-disc precession in UX Ursae Majoris
5. Arbitrarily Degenerate Helium White Dwarfs as Donors in AM Canum Venaticorum Binaries
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1. Evolutionary Period Changes for 52 Cataclysmic Variables, and the Failure for the Most-fundamental Prediction of the Magnetic Braking Model;The Astrophysical Journal;2024-05-01
2. An eclipsing 47 min double white dwarf binary at 400 pc;Monthly Notices of the Royal Astronomical Society;2023-08-04
3. Orbital Decay in an Accreting and Eclipsing 13.7 Minute Orbital Period Binary with a Luminous Donor;The Astrophysical Journal Letters;2023-08-01
4. Probing the Efficiency of Tidal Synchronization in Outspiralling Double White Dwarf Binaries with LISA;The Astrophysical Journal;2023-06-01
5. Spectroscopy of the helium-rich binary ES Ceti reveals accretion via a disc and evidence of eclipses;Astronomy & Astrophysics;2021-01
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