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Interpretation of Radio Observations of FH Serpentis
Published online by Cambridge University Press: 12 April 2016
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Seaquist and Palimaka (1977) interpreted the radio observations of this nova according to a “Hubble flow” model, in which all gas was ejected at the same time, and for which the velocity of any point in the shell at a given time is proportional to its radial distance. Their model involving a thick shell contradicts observations made in other parts of the spectrum of this and other novae, so in the present study other possibilities have been examined.
- Type
- Abstracts of Workshop Papers on Novae
- Information
- International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 523
- Copyright
- Copyright © The University of Rochester 1979
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