The little bang: Peculiarities in the local group and some dynamical explanations

Details The little bang: Peculiarities in the local group and some dynamical explanations The little bang: Peculiarities in the local group and some dynamical explanations

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aipc..336..450v&link_type=abstract

Dark matter. AIP Conference Proceedings, Volume 336, pp. 450-453 (1995).

Computer Science

5

Dark Matter, Background Radiations

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. We find 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 8 billion years ago.

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