Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-19T15:30:06.986Z Has data issue: false hasContentIssue false
  • English
  • Français

A New Estlmate of the Hubble Constant Using the Virgo Cluster Distance

Published online by Cambridge University Press:  25 April 2016

N. Visvanathan
N. Visvanathan*
Affiliation:
Mount Stromlo and Siding Spring Observatories, ANU
Get access Rights & Permissions [Opens in a new window]

Abstract

A new distance modulus (31.23) to the Virgo cluster is derived using the distances to nearby galaxies given by Sandage and Tammann, de Vaucouleurs, ourselves and DDO observers. This when combined with the undisturbed mean Virgo cluster velocity 1182 km s-1, gives a value for the global Hubble constant as 67 ±4 km s-1Mpc-1.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 2 , 1985 , pp. 140 - 144
Copyright
Copyright © Astronomical Society of Australia 1985

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Arnett, W. D., Branch, D., and Wheeler, C., 1985, Nature, 314, 337.Google Scholar
Caldwell, J. A. R., 1983, Observatory, 103, 244.Google Scholar
de Vaucouleurs, G., 1978, Astrophys. J., 223, 351.CrossRefGoogle Scholar
de Vaucouleurs, G., 1978a, Astrophys. J., 223, 730.CrossRefGoogle Scholar
de Vaucouleurs, G., 1978b, Astrophys. J., 224, 710.Google Scholar
de Vaucouleurs, G., 1982, Proc. Astron. Soc. Aust., 4, 320.Google Scholar
Dressier, A., 1984, Astrophys. J., 281, 512.CrossRefGoogle Scholar
Florentin-Nielsen, R., 1984, Astron. Astrophys., 138, L19.Google Scholar
Gregory, S. A., and Tifft, W. G., 1976, Astrophys. J., 205, 716.Google Scholar
Madore, B. F., 1982, Astrophys. J. (Letters), 257, L33.Google Scholar
Madore, B. F., 1985, Proceedings of IAU Colloquium #82, ‘Cepheids’: Observations and Theory’, Toronto, May, 1984.Google Scholar
Mathewson, D. S., Ford, V. L., Visvanathan, N., 1985, in preparation.Google Scholar
McGonegal, R., McLaren, R. A., McAlary, C. W., and Madore, B. F., 1982, Astrophys. J. (Letters), 257, L33.Google Scholar
McGonegal, R., McAlary, C. W., McLaren, R. A., and Madore, B. F., 1983, Astrophys. J., 269, 641.Google Scholar
Sandage, A., and Tammann, G. A., 1971, Astrophys. J., 167, 293.Google Scholar
Sandage, A., and Tammann, G. A., 1984, Nature, 307, 326.CrossRefGoogle Scholar
Tammann, G. A., and Sandage, A., 1984, preprint of the Astronomical Institute of the University of Basel, No. 6.Google Scholar
van den Bergh, S., 1977, IAU Coll. 37, CNRS Coll. No. 263.Google Scholar
Visvanathan, N., 1972, Pubi. Astron. Soc. Pacific, 84, 248.Google Scholar
Visvanathan, N., and Sandage, A., 1977, Astrophys. J., 216, 214.CrossRefGoogle Scholar
Visvanathan, N., 1983, Astrophys. J., 275, 430.Google Scholar
Visvanathan, N., 1985, Astrophys. J., 288, 182.CrossRefGoogle Scholar