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Extremely Slow Nova PU Vulpeculae - Seven Fat Years After Maximum

Published online by Cambridge University Press:  12 April 2016

D. Chochol  and
J. Grygar
D. Chochol
Affiliation:
Astronomical Institute, Slovak Academy of Sciences Tatranská Lomnica, Czechoslovakia
J. Grygar
Affiliation:
Astronomical Institute, Slovak Academy of Sciences Tatranská Lomnica, Czechoslovakia

Abstract

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UBV photometry and spectroscopy of the symbiotic nova PU Vul support the suggestion that the system consists of a mass-losing M-giant massive component and a C-O dwarf accreting hydrogen-rich matter, mimicing in outer appearance an F-supergiant.

Type
V. Nova and Dwarf Nova Outbursts
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 487 - 491
Copyright
Copyright © Reidel 1987

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