Bipolar radio sources in star-forming regions?

Details Bipolar radio sources in star-forming regions? Bipolar radio sources in star-forming regions?

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...248..221h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 1, Aug. 1991, p. 221-226.

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Herbig-Haro Objects, Pre-Main Sequence Stars, Radio Sources (Astronomy), Star Formation, Astronomical Models, Computational Astrophysics, Oblique Shock Waves, Particle Acceleration, Relativistic Particles

Scientific paper

A possible new type of behavior associated with the young stellar bipolar outflow sources is examined with particular reference to a triple radio source in Serpens. It is shown that the existence of bipolar nonthermal radio sources associated with outflows in star-forming regions is consistent with the current knowledge of these sources and of the theory of diffusive shock acceleration of relativistic particles. A criterion is presented for determining when the source may be dominated by thermal emission. Both thermal and nonthermal bipolar continuum radio sources in bipolar flows can thus be anticipated.

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