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Extremely Slow Nova PU Vulpeculae - Seven Fat Years After Maximum
Published online by Cambridge University Press: 12 April 2016
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
- Copyright
- Copyright © Reidel 1987
References
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