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Five Crucial Tests of the Cosmic Distance Scale Using the Galaxy as Fundamental Standard

Published online by Cambridge University Press:  25 April 2016

G. de Vaucouleurs
G. de Vaucouleurs*
Affiliation:
Mount Stromlo and Siding Spring Observatories, A.N.U.
*
*Visiting Fellow 1981-82, on leave from the University of Texas at Austin
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Extract

The traditional approach to the extragalactic distance scale rests on a pyramid of primary, secondary and tertiary indicators of increasing range and decreasing accuracy. This multi-step procedure, fraught with the danger of cumulative errors, has led in recent years to two main, widely diverging scales: the ‘long’ scale (Sandage and Tammann 1974, 1975, 1976) implying a Hubble constant and the ‘short’ scale (de Vaucouleurs 1978, 1979; de Vaucouleurs and Bollinger 1979; de Vaucouleurs and Peters 1981; de Vaucouleurs et al. 1981) leading to H0 ≃ 100. Several authors have already shown that the long scale rests on very precarious foundations (Capaccioli and Fasano 1980, de Vaucouleurs 1981, Hanes 1980); counter arguments have been offered in its defence and to criticize the short scale (Tammann, Sandage and Yahil 1979, Sandage and Tammann 1982). For want of a conclusive test a consensus was still lacking.

Type
Invited Papers
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 4 , 1982 , pp. 320 - 327
Copyright
Copyright © Astronomical Society of Australia 1982

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References

Aaronson, M., Huchra, J.P., and Mould, J.R., Astrophys. J., 229, 1 (1979)CrossRefGoogle Scholar
Aaronson, M. Mould, J.R., and Huchra, J.P., Astrophys. J., 237, 655 (1980).CrossRefGoogle Scholar
Aaronson, M. et al., Astrophys. J., 239, 12 (1980).CrossRefGoogle Scholar
Bancall, J.N., and Soneira, R.M., Astrophys. J. Suppl., 44, 73 (1980).CrossRefGoogle Scholar
Bottinelli, L., Gougenheim, L., Paturel, G., and de Vaucouleurs, G., Astrophys. J. (Letters), 242, L153 (1980).CrossRefGoogle Scholar
Capaccioli, M., and Fasano, G.,Astron. Astrophys., 83, 354 (1980).Google Scholar
de Vaucouleurs, G., Astrophys. J. Suppl., 6, 213 (1961).CrossRefGoogle Scholar
de Vaucouleurs, G. Astrophys. J. Suppl., 6, 213 (1980).CrossRefGoogle Scholar
de Vaucouleurs, G., IAU Symposium No. 38, p. 18 (1970).Google Scholar
de Vaucouleurs, G., ‘The Evolution of Galaxies and Stellar Populations’ P. 43, Yale Univ. Obs., New Haven (1977).Google Scholar
de Vaucouleurs, G., Astrophys. J., 223, 351, 730; 224, 14, 710 (1978).CrossRefGoogle Scholar
de Vaucouleurs, G., Astrophys. J., 227, 380, 729 (1979).CrossRefGoogle Scholar
de Vaucouleurs, G., Tenth Texas Symposium on Relativistic Astrophysics, p.90, New York Acad. Sci., New York (1981).Google Scholar
de Vaucouleurs, G., Astrophys. J., 253, 520 (1982).CrossRefGoogle Scholar
de Vaucouleurs, G., and Bollinger, G., Astrophys. J., 233, 433 (1979).CrossRefGoogle Scholar
de Vaucouleurs, G., de Vaucouleurs, A., and Corwin, H.G., Second Reference Catalogue of Bright Galaxies, Univ. of Texas Press (1976).Google Scholar
de Vaucouleurs, G., and Olson, D.W., Astrophys. J., in press (1982).Google Scholar
de Vaucouleurs, G., and Pence, W.D., Astron. J., 83, 1163 (1978).CrossRefGoogle Scholar
de Vaucouleurs, G., and Peters, W.L., Astrophys. J., 248, 395 (1981).CrossRefGoogle Scholar
de Vaucouleurs, G., Peters, W.L., Bottinelli, L., Gouguenheim, L., and Paturel, G., Astrophys. J., 248, 408 (1981).CrossRefGoogle Scholar
Faber, S.M., and Jackson, R.E., Astrophys. J., 204, 668 (1976).CrossRefGoogle Scholar
Fliche, H.H., and Souriau, J.M., Astron. Astrophys., 78, 87 (1979).Google Scholar
Hanes, D.A., Mon. Not. R. Astron. Soc, 180, 309 (1977).CrossRefGoogle Scholar
Hanes, D.A., Mon. Not. R. Astron. Soc, 188, 901 (1979).CrossRefGoogle Scholar
Hanes, D.A., Anglo Austr. Observ. Preprint No. 140 (1980).Google Scholar
Paturel, G., Thesis, Univ. of Lyon (1981) and Astron. Astrophys. in press (1982).Google Scholar
Sandage, A., and Tammann, G.A., Astrophys. J., 190, 525; 191, 603;194, 223, 559 (1974).CrossRefGoogle Scholar
Sandage, A., and Tammann, G.A., Astrophys. J., 196, 313; 197, 265 (1975).CrossRefGoogle Scholar
Sandage, A., and Tammann, G.A., Astrophys. J., 210, 7 (1976).CrossRefGoogle Scholar
Sandage, A., and Tammann, G.A., A Revised Shapley-Ames Catalogue of Bright Galaxies, Carnegie Inst. Publ. 695 (1981).Google Scholar
Sandage, A., and Tammann, G.A., Astrophysical Cosmology, Vatican Study Week, in press (1982).Google Scholar
Simien, F., and de Vaucouleurs, G., IAU Symposium No. 100, Besancon, submitted (1982).Google Scholar
Tammann, G.A., Sandage, A., and Yahil, A., Physical Cosmology, p. 53, Les Houches, Sess. XXXII; North Holland, Amsterdam (1979).Google Scholar
Tully, R.B., and Fisher, A., Astron. Astrophys., 54, 661 (1977).Google Scholar
van den Bergh, S., The Galaxies of the Local Group, Comm. David Dunlap Obs. No. 195 (1968).Google Scholar
Whitmore, B.C., Kirshner, R.P., and Schechter, P.L., Astrophys. J., 234, 68 (1979).CrossRefGoogle Scholar
Whitmore, B.C., and Kirshner, R.P., Astrophys. J., 250, 43 (1981).CrossRefGoogle Scholar