Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...260...17t&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 260, no. 1-2, p. 17-32.
Astronomy and Astrophysics
Astronomy
36
Galactic Structure, Local Group (Astronomy), Velocity Distribution, Virgo Galactic Cluster, Astronomical Models, Hubble Constant
Scientific paper
Results are presented of an investigation of the velocity-distance relation close to the direction of the Virgo cluster, with distances from the Tully-Fisher relation, and with attention to the Malmquist bias. For Theta greater than 8 deg, a behavior is revealed which is as expected Tolman-Bondi solutions for an expanding spherical mass distribution. Various density distributions, constrained by the mass inside the Local Group distance, agree with the observations, but only if the mass within the Virgo 6 deg region is close to or larger than the standard Virgo virial mass values. It is inferred that the central 6-degree mass has the standard M (virial) as a rough lower limit. From this it follows, together with the light ratios within the local supercluster and the light enhancement relative to the general field, that light does not trace mass. Background contamination produces an asymmetrical distribution of velocities behind r(Vir).
Bottinelli Lucette
Gouguenheim Lucienne
Paturel Georges
Teerikorpi Pekka
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