On the Motion in the Local Group of Galaxies

Details On the Motion in the Local Group of Galaxies On the Motion in the Local Group of Galaxies

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..895..321n&link_type=abstract

FIFTY YEARS OF ROMANIAN ASTROPHYSICS. AIP Conference Proceedings, Volume 895, pp. 321-324 (2007).

Astronomy and Astrophysics

Astrophysics

Galaxy Clusters

Scientific paper

The authors study the Local Group of Galaxies approximating it as a
binary galaxy (Milky Way and Andromeda Nebula). They find that inside
100 kpc from the Milky-Way centre the influence of the Andromeda Nebula
is very weak and that for the satellites of the Milky Way, even for the
outer ones, perigalactic distances of about 30-40 kpc are likely.

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