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Radiation Pressure in Nova Ejecta

Published online by Cambridge University Press:  12 April 2016

James W. Younger
James W. Younger*
Affiliation:
Department of Astronomy, Indiana University

Extract

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The main features of the spectral evolution of novae consist of: 1. An overall increase in absorption line velocities and emission line widths as a function of time past maximum light. 2. The subsequent appearance of an absorption line system at roughly twice the velocity of the previous absorption line system. 3. Some absorption line systems apparently consist of multiple absorption components at different velocities.

Type
Abstracts of Workshop Papers on Novae
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 527
Copyright
Copyright © The University of Rochester 1979

References

Rybicki, G.B., and Hummer, D.G. 1978, Ap.J., 219, 654.Google Scholar