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Supernovae and Cosmology

Published online by Cambridge University Press:  30 March 2016

Norbert Bartel*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, U.S.A.

Abstract

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I review the presently existing four partly independent methods of determining extragalactic distances through supernova investigations and conclude that, although each of these methods has its difficulties, application of all of them on the same class of objects provides the opportunity of obtaining unique redundancy in determinations of extragalactic distances and Hubble’s constant.

Type
Joint Discussions
Copyright
Copyright © Reidel 1986

References

REFERENCES

Aaronson, M., Huchra, J., Mould, J., Schechter, P.L., and Tully, R.B. 1982, Ap. J., 258, 64.CrossRefGoogle Scholar
Arnett, W.D., Branch, D., and Wheeler, J.C. 1985, Nature, 814, 337.CrossRefGoogle Scholar
Baade, W. 1926, Astr. Nachr., 228, 359.CrossRefGoogle Scholar
Bandiera, R., Pacini, F., and Salvati, M. 1983, Astr. Ap., 126, 7.Google Scholar
Bartel, N. 1985, in Supernovae as Distance indicators, Lecture Notes in Physics, ed. Bartel, N. (Springer-Verlag, Berlin), 224, 107.CrossRefGoogle Scholar
Bartel, N., Rogers, A.E.E., Shapiro, I.I., Gorenstein, M.V., Gwinn, C.R., Marcaide, J.M., and Weiler, K.W. 1985, Nature, 318, 25.CrossRefGoogle Scholar
Branch, D., Falk, S.W., McCall, M.L., Rybski, P., Uomoto, A., and Wills, B.J. 1981, Ap. J., 244, 780.CrossRefGoogle Scholar
Branch, D. and Patchett, B. 1973, M. N. R. A. S., 161, 71.CrossRefGoogle Scholar
Cadonau, R., Sandage, A., and Tammann, G.A. 1985, in Supernovae as Distance Indicators, Lecture Notes in Physics, ed. Bartel, N. (Springer-Verlag, Berlin), 224, 151.CrossRefGoogle Scholar
Chevalier, R.A. 1982, Ap. J., 259, 302.CrossRefGoogle Scholar
Chevalier, R.A. 1986, this volume.Google Scholar
de Vaucouleurs, G. and Bollinger, G. 1979, Ap. J., 233, 433.CrossRefGoogle Scholar
de Vaucouleurs, G. and Corwin, H.G. Jr., 1985, Ap. J., 297, 23.CrossRefGoogle Scholar
Fransson, C. 1986, this volume.Google Scholar
Hershkowitz, S., Linder, E., and Wagoner, R.V. 1986, Ap. J., 301, 220.CrossRefGoogle Scholar
Huchra, J.P. 1985, in The Virgo Cluster, eds. Richter, O.-G. and Binggeli, B., ESO proc. 20, 181.Google Scholar
Kirshner, R.P. and Kwan, J. 1974, Ap. J., 193, 27.CrossRefGoogle Scholar
Kowal, C.T. 1968, A. J., 73, 1021.CrossRefGoogle Scholar
Marscher, A.P. 1985, in Supernovae as Distance Indicators, Lecture Notes in Physics, ed. Bartel, N. (Springer-Verlag, Berlin), 224, 130.CrossRefGoogle Scholar
Panagia, N. 1985, in Supernovae as Distance Indicators, Lecture Notes in Physics, ed. Bartel, N. (Springer-Verlag, Berlin), 224, 14.CrossRefGoogle Scholar
Sandage, A., and Tammann, G.A. 1985, in Supernovae as Distance Indicators, Lecture Notes in Physics, ed. Bartel, N. (Springer-Verlag, Berlin), 224, 1.CrossRefGoogle Scholar
Shaviv, G., Wehrse, R., and Wagoner, R.V. 1985, Ap. J., 289, 198.CrossRefGoogle Scholar
Uomoto, A., and Kirshner, R.P. 1985, Astr. Ap., 149, L7.Google Scholar
Wagoner, R.V. 1981, Ap. J. (Lett.), 250, L65.CrossRefGoogle Scholar
Weiler, K.W., Sramek, R.A., Panagia, N., van der Hulst, J.M., and Salvati, M. 1986, Ap. J., 301, 790.CrossRefGoogle Scholar
Wesselink, A.J. 1946a, B.A.N., 10, 83.Google Scholar
Wesselink, A.J. 1946b, B.A.N., 10, 251.Google Scholar
Wesselink, A.J. 1985, in Supernovae as Distance Indicators, Lecture Notes in Physics, ed. Bartel, N. (Springer-Verlag, Berlin), 224, 166.CrossRefGoogle Scholar
Wheeler, J.C., and Levreault, R. 1985, Ap. J. (Lett.), 294, L17.CrossRefGoogle Scholar