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On possible mass loss from the supergiant RHO Cassiopeia

Published online by Cambridge University Press:  12 April 2016

M. Boyarchuk
M. Boyarchuk*
Affiliation:
Crimean Astrophysical Observatory

Extract

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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