Abstract
The good agreement found between the observed flux of radio emission of the Nova Delphini 1967 and that calculated theoretically enables us to deduce the angular diameter of the Nova's envelope. This result, when combined with the known linear diameter of the envelope, gives a distance of the order of 885 pc for Nova Delphini.
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Andrillat, Y. et Houziaux, L.: 1971,Astrophys. Space Sci. 13, 100.
Barnes, T., Van den Bergh, S., Hagen, G., Jackson, P., Racine, R., Remage, N., et Watte, V.: 1967,J. Roy. Astron. Soc. Canada 61, 339.
Fehrenbach, Ch. et Petit, M.: 1968,Astron. Astrophys. 1, 403.
Garstang, R. H.: 1968, in D. J. Osterbrock and C. R. O'Dell (eds.), ‘Planetary Nebulae’,IAU Symp. 34, 143.
Hutchings, J. B.: 1968, in M. Hack (ed.),Mass Loss From Stars, D. Reidel Publ. Co., Dordrecht, p. 290.
Hjellming, R. M. et Churchwell, E.: 1968,Astrophys. Letters 4, 165.
Hjellming, R. M. et Wade, C. M.: 1970,Astrophys. J. (Letters) 162, L1.
Khromov, G. S.: 1968,Mem. Soc. Roy. Sci. Liège, 5ème série, tom. 17, 289.
Malakpur, I.: 1973a,Astron. Astrophys. 24, 125.
Malakpur, I.: 1973b,Astron. Astrophys. 28, 393.
Malakpur, I.: 1974, Soumis àAstron. Astrophys.
Monnery, E. J.: 1970,Publ. Astron. Soc. Pacific 82, 626.
Smith, K., Henry, R. J. W., et Burke, P. G.: 1967,Phys. Rev. 157, 51.
Zellner, B. et Morrison, N. O.: 1971,Astron. J. 76, 645.
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Malakpur, I. La distance de la Nova Delphini 1967. Astrophys Space Sci 38, 403–406 (1975). https://doi.org/10.1007/BF00647141
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DOI: https://doi.org/10.1007/BF00647141