Peculiarities in the Local Group of galaxies and some dynamical explanations.

Details Peculiarities in the Local Group of galaxies and some dynamical explanations. Peculiarities in the Local Group of galaxies and some dynamical explanations.

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992amfa.meet....1v&link_type=abstract

Annual meeting of the Finnish Astronomical Society, p. 1 - 10

Astronomy and Astrophysics

Astronomy

Scientific paper

There has been increasing evidence that Maffei 1/2 and IC 342 are close to the Local Group of galaxies, so close that they have to be included in the discussion of the history of group. The authors found that the dynamical evolution in the local area may have been quite complicated in comparison with the traditional Kahn-Woltjer model. For example, the Andromeda galaxy may be a product of a merger of two major galaxies, and Maffei 1/2 and IC 342 may have been thrown out of the Local Group about 6 billion years ago.

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