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A Model of Nova Delphini 1967 from its Nebular Spectrum

Published online by Cambridge University Press:  12 April 2016

Waltraut Carola Seitter

Extract

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Nova Delphini 1967 is outstanding among other recent novae since it belongs to the rare class of extremely slow objects. Another unusual characteristic is the pronounced pattern of the emission lines during the nebular stage.

Type
IV. Duplicity and its Consequences among the Intrinsic Variable Stars
Information
International Astronomical Union Colloquium , Volume 15: New Directions and Frontiers in Variable Stars Research , 1971 , pp. 268 - 274
Copyright
Copyright © Cambridge University Press 1971

References

Andrillat, Y., and Houziaux, L., 1969, in „Mass Loss from Stars“, ed. by Hack, M., p. 281.Google Scholar
Mustel, E. R. and Boyarchuk, A. A., 1970, Astrophys. and Space Sc. 6, p. 183.CrossRefGoogle Scholar
Payne-Gaposchkin, C., 1964, „The Galactic Novae“, p. 62 (Dover).Google Scholar
Herczeg, T., 1958, Memorie Soc. Astr. Ital. Vol XXIX, p. 1.Google Scholar
Wenzel, W., 1971, private communication.Google Scholar