Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-20T05:19:25.477Z Has data issue: false hasContentIssue false
  • English
  • Français

Element Abundance Analyses of Novae

Published online by Cambridge University Press:  12 April 2016

Robert E. Williams
Robert E. Williams*
Affiliation:
Steward Observatory, University of Arizona, Tucson, ArizonaUSA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The different methods by which element abundances in novae have been determined are reviewed. Curve of growth studies of novae at maximum light have indicated CNO nuclei to be greatly enhanced with respect to hydrogen in certain objects. These results are questionable because they depend upon an assumed temperature distribution in the photosphere which is probably too steep to be realistic. Emission line analyses of novae, generally obtained in the period of early decline, also indicate possible heavy element enhancement, however these results are tentative because of uncertainties in the parameters of the emitting gas. It is suggested that useful abundance determinations of nova ejecta might be obtained from studies of old, extended nova shells.

Type
Part II: Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 42: The Interaction of Variable Stars with their Environment , 1977 , pp. 242 - 273
Copyright
Copyright © Veröff. Der Remeis-Sterwarte 1977

References

Andrlllat, Y., and Collin-Souffrin, S. 1974, Astron. and Ap., 31, 347.Google Scholar
Antipova, L. I. 1971, Soviet Astron. - AJ, 15, 225.Google Scholar
Antipova, L. I. 1974, in Highlights of Astronomy, ed. Contopoulos, G. (Dordrecht: Reidel Publ. Co.), 3, 501.CrossRefGoogle Scholar
Black, J. H., and Gallagher, J. S. 1976, Nature, 261, 296.Google Scholar
Collin-Souffrin, S. 1977, in Novae and Related Objects, ed. Friedjung, M. (Dordrecht: Reidel Publ. Co.).Google Scholar
Doroshenko, V. T. 1968, Soviet Astron. - AJ, 12, 95.Google Scholar
Fehrenbach, C., and Andrillat, Y. 1976, Astron. and Ap., 52, 123.Google Scholar
Ferland, G. J. 1977, Ap. J., in press.Google Scholar
Ferland, G., Lambert, D. L., and Woodman, J. H. 1977, Ap. J., 213, 132.Google Scholar
Gallagher, J. S. 1977, Ap. J., in press.Google Scholar
Gallagher, J. S., and Anderson, C. M. 1976, Ap. J., 203, 625.Google Scholar
Grasdalen, G. L., and Joyce, R. R. 1976, Nature, 259, 187.Google Scholar
Greenstein, J. L. 1948, Ap. J., 107, 151.Google Scholar
Greenstein, J. L., and Kraft, R. P. 1959, Ap. J., 130, 99.Google Scholar
Hutchings, J. B. 1972, MNRAS, 158, 177.Google Scholar
Kaler, J. B. 1976, Ap. J. Suppl., 31, 517.Google Scholar
Kraft, R. P. 1959, Ap. J., 130, 110.Google Scholar
Malakpur, I. 1973, Astron. and Ap., 24, 125.Google Scholar
McLaughlin, D. B. 1937, Pub. Obs. Mich., 6, 107.Google Scholar
McLaughlin, D. B. 1944, Pub. Obs. Mich., 8, 149.Google Scholar
McLaughlin, D. B. 1960, in Stellar Atmospheres, ed. Greenstein, J. L. (Chicago: Univ. of Chicago Press), p. 585.Google Scholar
Mihalas, D. 1970, Stellar Atmospheres (San Francisco: W. H. Freeman), p. 337.Google Scholar
Mustel, E. R. 1974, in Vistas in Astronomy, ed. Beer, A. (Oxford: Pergamon), 16, 260.Google Scholar
Mustel, E. R., and Antipova, L. I. 1971, Nauch. Inform. Moscow, 19, 32.Google Scholar
Mustel, E. R., and Baranova, L. I. 1965, Soviet Astron. - AJ, 9, 31 Google Scholar
Mustel, E. R., and Boyarchuk, A. A. 1970, Ap. and Sp. Sci., fr, 183.Google Scholar
Mustel, E. R., and Boyarchuk, M. E. 1959, Soviet Astron. - AJ, 3, 744.Google Scholar
Osmer, P. S. 1972, Ap. J. Suppl., 24, 255.Google Scholar
Parsons, S. B. 1967, Ap. J., 150, 263.Google Scholar
Payne-Gaposchkln, C. 1957, The Galactic Novae (Amsterdam: North-Holland Publ. Co.).Google Scholar
Pottasch, S. R. 1959, Ann. d’Ap., 22, 412.Google Scholar
Pottasch, S. R. 1967, B. A. N. 19, 227.Google Scholar
Ruusalepp, M., and Luud, L. 1970, Publ. Tartu Obs., 39, 89.Google Scholar
Searle, L., Sargent, W. L. W., and Jugaku, J. 1963, Ap. J., 137, 268.Google Scholar
Sneden, C., and Lambert, D. L. 1975, MNRAS, 170, 533.Google Scholar
Soderblom, D. 1976, Pub. Ast. Soc. Pac, 88, 517.Google Scholar
Sparks, W. H., and Starrfield, S. 1973, MNRAS, 164, IP.CrossRefGoogle Scholar
Starrfleld, S. G., Truran, J. W., and Sparks, W. M. 1977, In CNO Isotopes In Astrophysics, ed. Audouze, J. (Dordrecht: Reidel Publ. Co.), p. 49.CrossRefGoogle Scholar
Strittmatter, P. A., Woolf, N. J., Thompson, R. I., Wilkerson, S., Angel, J. R. P., Stockman, H. S., Gilbert, G., Grandi, S. A., Larson, H., and Fink, V. 1977, Ap. J., in press.Google Scholar
Walker, M. F. 1954, Pub. Ast. Soc. Pac, 6, 230.Google Scholar
Weaver, H. F. 1974, in Highlights of Astronomy, ed. Contopoulos, G. (Dordrecht: Reidel Publ. Co.), 3, 509.CrossRefGoogle Scholar
Yamashita, Y. 1975, Ann. Tokyo Obs., 15, 1.Google Scholar