Abstract
Infrared spectra at 39 Å/mm of Nova Delphini 1967 have been obtained in the wavelength range λ 6500– λ 8800. Typical microphotometer tracings are displayed and an estimate of the received flux is given for the most prominent lines at nebular stage. Loss of matter is very likely to occur.
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References
Andrillat, Y.: 1963, Colloque sur les novae, les novoïdes et les supernovae, Paris, CNRS, 1964, p. 136.
Andrillat, Y. and Houziaux, L.: 1967, in IAU Symposium No. 34: Planetary Nebulae (ed. by D. E. Osterbrock), D. Reidel Publ. Co., Dordrecht, p. 68.
Fehrenbach, C., Andrillat, Y. and Bloch, M.: 1967, C. R. Acad. Sc. Paris 266, 106; 1968, 265, 583.
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© 1969 D. Reidel Publishing Company, Dordrecht, Holland
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Andrillat, Y., Houziaux, L. (1969). Infrared Spectra of Nova Delphini 1967. In: Hack, M. (eds) Mass Loss from Stars. Astrophysics and Space Science Library, vol 13. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3405-0_38
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DOI: https://doi.org/10.1007/978-94-010-3405-0_38
Publisher Name: Springer, Dordrecht
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