M87 - Round and slow

Details M87 - Round and slow M87 - Round and slow

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...290...94d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 290, March 1, 1985, p. 94, 95.

Astronomy and Astrophysics

Astrophysics

5

Galactic Radiation, Galactic Structure, Radio Spectra, X Ray Sources, Astrodynamics, Density Distribution, Gas Flow, H Beta Line, High Temperature Gases, Temperature Profiles

Scientific paper

The authors show that the X-ray emitting gas in M87 is flowing through
the galaxy at less than 10 km s-1. This rules out models in
which motion of the gas explains the asymmetric radio continuum and
Hβ emission in the central regions.

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