No CrossRef data available.
Article contents
Mass ejections from the G-type hypergiant HR 8752
Published online by Cambridge University Press: 12 April 2016
Extract
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