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First Measurements of γ Cassiopeae's Hydrogen Envelope
Published online by Cambridge University Press: 23 September 2016
Extract
In the framework of an interferometric program on Be stars, first announced during the IAU general assemblies at Patras, 1982, recently at New Delhi, 1985 and reported in the “Be Star Newsletter” n°6 and l3, we try to measure the angular diameter of the central star, hydrogen envelope and, if possible, its movement, of the brightest Be stars in the context of pulsating atmosphere or binary star hypothesis.
- Type
- IIA. The Underlying Stars: Observations
- Information
- International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 66 - 67
- Copyright
- Copyright © Cambridge University Press 1987