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Mass ejections from the G-type hypergiant HR 8752

Published online by Cambridge University Press:  12 April 2016

J. Smoliński ,
J.L. Climenhaga  and
J.M. Fletcher
J. Smoliński
Affiliation:
N. Copernicus Astronomical Center, Toruń, Poland
J.L. Climenhaga
Affiliation:
N. Copernicus Astronomical Center, Toruń, Poland
J.M. Fletcher
Affiliation:
Dominion Astrophysical Observatory, Victoria, BC, Canada

Extract

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One of the most luminous stars in our Galaxy (Humphreys 1988) HR 8752 = HD 217476 (G0 Ia), is similar in some respects to Luminous Blue Variables. Studies by several authors (Sargent 1965; Smoliński 1971; Smoliński et al. 1977; Stickland and Harmer 1978; Lambert and Luck 1978; Lambert et al. 1981; Smoliński et al. 1986; Sheffer and Lambert 1987) have contributed to the understanding of activities in the atmosphere of this star, but its nature is still not well understood.

Type
Section I: Main Papers, General Discussions, and Two Panel Discussions
Information
International Astronomical Union Colloquium , Volume 113: Physics of Luminous Blue Variables , 1989 , pp. 131 - 134
Copyright
Copyright © Kluwer 1989

References

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