The peculiar interacting binary V Sagittae: Brightness variations in 1932 – 1994
Astron. Astrophys. Suppl. Ser., 118 3 (1996) 421-428
Published online: 1996-09-15
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A Limit Cycle Model For Long‐Term Optical Variations of V Sagittae: The Second Example of Accretion Wind Evolution
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Orbital Light Curve of the Peculiar Binary V Sagittae in ExtendedHigh States of Brightness
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Time‐resolved Spectroscopy of V Sagittae
Marcos P. DiazPublications of the Astronomical Society of the Pacific 111 (755) 76 (1999)
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The V Sagittae Stars
J. E. Steiner and M. P. DiazPublications of the Astronomical Society of the Pacific 110 (745) 276 (1998)
https://doi.org/10.1086/316139