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=1986cha%26a..10..217x&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 10, Issue 3, p. 217-220.

Astronomy and Astrophysics

Astrophysics

3

Galaxies - Radio Galaxies

Scientific paper

Results of our wide beam radio observations of M87 are given here. Combined with the infrared observations of Virgo (Ceccarelli et al. 1982), we show that in order to explain both the radio and infrared observations, it is convenient to postulate an extended tepid (~(+5)K) halo, in addition to a hot (~(+8)K) halo surrounding M87. This tepid halo would be able to close the system gravitationally.

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