A model of the radio continuum filaments in the galactic center

Details A model of the radio continuum filaments in the galactic center A model of the radio continuum filaments in the galactic center

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...288..377q&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 288, Jan. 1, 1985, p. 377-384.

Astronomy and Astrophysics

Astronomy

22

Filaments, Galactic Nuclei, Milky Way Galaxy, Radio Sources (Astronomy), Astronomical Maps, Gravitational Effects, Interstellar Matter, Many Body Problem, Nebulae, Particle Trajectories

Scientific paper

High-resolution radio continuum studies of the galactic center have revealed several spiral-like structures within the central 2 pc. The authors show that one of these structures can be modeled as the infall and tidal breakup of a small molecular cloud under the influence of the gravitational field of the center of the galaxy and a dissipative medium. The derived model parameters and model geometry imply the ejection of material near the escape velocity and the existence of a diffuse interstellar medium with a temperature of order 106K.

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