On the mass of the Local Group

Details On the mass of the Local Group On the mass of the Local Group

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87..827h&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 87, Oct. 1975, p. 827-829. Research supported by the National Research C

Astronomy and Astrophysics

Astronomy

2

Andromeda Galaxy, Angular Velocity, Galactic Clusters, Galactic Rotation, Local Group (Astronomy), Mass Distribution, Astronomical Models, Internal Energy, Magellanic Clouds, Spatial Distribution

Scientific paper

The effect of varying the rotation velocity of the local standard of
rest on the stability of the Local Group is investigated. It is
concluded that, unless the rotation velocity of the local standard of
rest is greater than about 290 km per sec, unseen mass is probably
required for stability.

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