Origin of the coronal lines of novae

Details Origin of the coronal lines of novae Origin of the coronal lines of novae

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72..143m&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 1, Sept. 1980, p. 143-157. In French.

Physics

Line Spectra, Novae, Stellar Coronas, Stellar Spectra, Forbidden Transitions, Stellar Envelopes, Theoretical Physics

Scientific paper

Lines identified in spectral region 3060-6100 A of the Nova Delphini 1967 are presented. The coronal lines of the novae Herculis 1960, Herculis 1963, Delphini 1967, Serpentis 1970, Scuti 1975, and Cygni 1975 are studied, and the observational results of these novae as well as those obtained for older novae and the recurrent nova RS Ophiuchi are given. It is found that the shock wave produced by the collision of the main envelope with the dusty circumstellar envelope heat the circumstellar envelope, and the heated material then emits the coronal lines.

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