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Hubble Constant in the Local Region

Published online by Cambridge University Press:  25 April 2016

N. Visvanathan
N. Visvanathan*
Affiliation:
Mount Stromlo and Siding Spring Observatories Australian National University
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Extract

One of the important discoveries of the present century is that the Universe expands. Two important parameters which define the dynamics of the Universe and can be obtained at the telescope are the rate of expansion zhqо, and change of this rate with time qо, It is difficult to derive a value for Hо because accurate distances of farther galaxies are needed. This involves identifying the luminous objects, such as brightest stars, HII regions, globular cluster, supernova etc., in the Local Group galaxies as well as in the external galaxies. Once the absolute magnitudes of these objects are calibrated with the known distances of the Local Group galaxies, distances to the external galaxies can be derived.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 5 , 1979 , pp. 309 - 311
Copyright
Copyright © Astronomical Society of Australia 1979

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References

Baum, W.A., Pub. A.S.P., 71, 106 (1959).CrossRefGoogle Scholar
de Vaucouleurs, G., in Vistas in Astronomy, Vol. 2, ed. Beer, A., (London: Pergammon Press), p. 1584 (1956).Google Scholar
de Vaucouleurs, G., Astro». J., 63, 253 (1958).CrossRefGoogle Scholar
de Vaucouleurs, G., Astrophys. J. Suppl., 5, 233 (1961).CrossRefGoogle Scholar
Faber, S.M., Astrophys. J., 179, 731 (1973). Gott, R.J., Gunn, J.E., Schramm, D.N., and Tinsley, B., Astrophys. J., 194, 543 (1974).CrossRefGoogle Scholar
Gunn, J.E., and Gott, J.R., Astrophys. J., 176, 1 (1972).CrossRefGoogle Scholar
Lasker, B.M., Astron. J., 75, 21 (1970).CrossRefGoogle Scholar
Peimbert, M., and Torres-Peimbert, S., Astrophys. J., 193, 327 (1974).CrossRefGoogle Scholar
Sandage, A., Astrophys. J., 202, 563 (1975).CrossRefGoogle Scholar
Sandage, A., and Tammann, G.A., Astrophys. J., 194, 559 (1974).CrossRefGoogle Scholar
Sandage, A., and Visvanathan, N., Astrophys. J., 223, 707 (1978).CrossRefGoogle Scholar
Visvanathan, N., Astron. Astrophys., 67, L17 (1978).Google Scholar
Visvanathan, N., Astrophys. J., 228, 81 (1979).CrossRefGoogle Scholar
Visvanathan, N., and Griersmith, D., Astrophys. J., 230, 1 (1979).CrossRefGoogle Scholar
Visvanathan, N., and Sandage, A., Astrophys. J., 216, 214 (1977).CrossRefGoogle Scholar