The V Sagittae Stars
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1538-3873/110/i=745/a=276/pdf
Reference48 articles.
1. A catalog of X-ray sources
2. CAL 87 - an eclipsing black hole binary?
3. CAL 83 - A puzzling X-ray source in the Large Magellanic Cloud
4. The Large Magellanic Cloud Supersoft X-Ray Binary RX J0513.9-6951
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1. Long-term spectral variations of V Sagittae: Two spectroscopic states with red- or blue-shifted emission wings of H i and He ii;Publications of the Astronomical Society of Japan;2024-08-16
2. 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
3. Accretion rates of 42 nova-like stars with IUE and Gaia data;Astronomy & Astrophysics;2024-01
4. An observed population of intermediate-mass helium stars that have been stripped in binaries;Science;2023-12-15
5. Revised ephemeris and orbital period derivative of the supersoft X-ray source CAL 87 based on 34 yr of observations;Monthly Notices of the Royal Astronomical Society;2023-11-27
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