Large beam radio observations of M87

Details Large beam radio observations of M87 Large beam radio observations of M87

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986acaps...6..119x&link_type=abstract

(Acta Astrophysica Sinica, vol. 6, 1986, p. 119-123) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 10, Sept. 1986, p

Astronomy and Astrophysics

Astronomy

Elliptical Galaxies, Radio Astronomy, Virgo Galactic Cluster, Halos, Interstellar Gas

Scientific paper

The authors show how combined large-beam infrared and radio observations
towards M87 may be explained by assuming the existence of a large
(105K) dark matter halo surrounding the giant galaxy M87. The
total mass of the more extended halo is 1013M_sun;. Such a
halo would be able to close the cluster gravitationally.

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