Hostname: page-component-848d4c4894-ttngx Total loading time: 0 Render date: 2024-05-16T22:34:53.519Z Has data issue: false hasContentIssue false
  • English
  • Français

Interpretation of Radio Observations of FH Serpentis

Published online by Cambridge University Press:  12 April 2016

M. Friedjung
M. Friedjung*
Affiliation:
Institut d’Astrophysique, Paris, France

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

References

Seaquist, E.R., and Palimaka, J. 1977, Ap.J., 217, 781.Google Scholar