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HM Sagittae: an eruptive variable resembling V1016 Cygni

Published online by Cambridge University Press:  12 April 2016

F. Ciatti ,
A. Mammano  and
A. Vittone
F. Ciatti
Affiliation:
Asiago Astrophysical Observatory
A. Mammano
Affiliation:
Asiago Astrophysical Observatory
A. Vittone
Affiliation:
Asiago Astrophysical Observatory

Extract

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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
International Astronomical Union Colloquium , Volume 42: The Interaction of Variable Stars with their Environment , 1977 , pp. 234 - 235
Copyright
Copyright © Veröff. Der Remeis-Sterwarte 1977

References

Dokuchaeva, O.D. 1976, Inf.Bull.Var.Stars No 1189 Google Scholar
Davidson, K., Humphreys, R.M., Merrill, K.M. 1977, PreprintGoogle Scholar
Feldman, P.A. 1977, IAU Circular No 3081 Google Scholar
Mammano, A., Ciatti, F. 1975, Astron.Astrophys. 39, 405 Google Scholar