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HM Sagittae: an eruptive variable resembling V1016 Cygni
Published online by Cambridge University Press: 12 April 2016
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We present photometric and spectroscopic observations (intermediate dispersion in the wavelength range 3700-10900 Å) of the recently discovered variable HM Sagittae (Dokuchaeva, 1976). Also pre-outburst data, indicating a red star, are used to discuss its nature and distance.
- Type
- Part II: Cataclysmic Variables
- Information
- Copyright
- Copyright © Veröff. Der Remeis-Sterwarte 1977
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