Inner rings in galaxies and the Hubble constant

Details Inner rings in galaxies and the Hubble constant Inner rings in galaxies and the Hubble constant

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986velen......121t&link_type=abstract

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia (ISSN 0024-0850), April 1986, p. 121, 122. In Russian.

Astronomy and Astrophysics

Astronomy

Galactic Structure, Hubble Constant, Ring Structures, Distance, Error Analysis, Galactic Clusters

Scientific paper

The method of Buta and de Vaucouleurs for determining the distance to galaxies, with inner ring structures used as distance indicators, is examined. It is noted that, in using this method, the Hubble constant should be estimated with allowance for the systematic error due to incomplete sampling. For five galaxy clusters, a Hubble constant value of 75 plus or minus 3 km/s/Mpc is obtained using de Vaucouleurs' local scale and a value of 58 km/s/Mpc is obtained using the scale of Sandage and Tammann.

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