The formation of the principal system of novae

Details The formation of the principal system of novae The formation of the principal system of novae

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...180..155f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 180, no. 1-2, June 1987, p. 155-159.

Astronomy and Astrophysics

Astrophysics

19

Absorption Spectra, Astronomical Models, Novae, Planetary Nebulae, Stellar Mass Ejection, Stellar Winds, Emission Spectra, High Temperature Plasmas, Stellar Coronas, X Ray Absorption, X Ray Sources

Scientific paper

The formation of the principal absorption system which appears to contain most of the mass ejected by a classical nova, can at least in some cases be explained by the collision of a high velocity wind responsible for the formation of spectrum line components belonging to the diffuse enhanced and Orion systems, with slower moving material associated with the pre-maximum system. Therefore the principal system can be explained in the framework of continued ejection in a similar way to that of the Kwok et al. (1978) theory for the formation of planetary nebulae. The presence of hot plasma is also predicted by this model.

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