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On possible mass loss from the supergiant RHO Cassiopeia
Published online by Cambridge University Press: 12 April 2016
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The supergiant Rho Cas F8Ia has a very high luminosity. Astronomers have payed attention to this star in August 1946, when its by its brightness had dropped from 4.2 to 6.2. The systematic spectrographic observations of Rho Cas are beeing carried out at the Crimean Astrophysical Observatory since 1965. No large light variations were observed during that time.
- Type
- Session II - Winds from Late Type Stars: Observations
- Information
- International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 117 - 118
- Copyright
- Copyright © Reidel 1981
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