Milli-arcsecond jets in radio galaxies - Interpretation

Details Milli-arcsecond jets in radio galaxies - Interpretation Milli-arcsecond jets in radio galaxies - Interpretation

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...254..465l&link_type=abstract

Astrophysical Journal, Part 1, vol. 254, Mar. 15, 1982, p. 465-471.

Astronomy and Astrophysics

Astrophysics

31

Galactic Radiation, Galactic Structure, Plasma Jets, Radio Galaxies, Synchrotron Radiation, Very Long Base Interferometry

Scientific paper

Some implications of observed parsec-scale jets in double radio galaxies
are considered. It is concluded that in all cases observed thus far, the
asymmetry reflects an intrinsic asymmetry on a parsec scale. If the jet
in Cyg A is pressure-confined, it must be surrounded by gas hotter than
50 million K.

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