Plasma processes in the excitation of Herbig-Haro objects

Details Plasma processes in the excitation of Herbig-Haro objects Plasma processes in the excitation of Herbig-Haro objects

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ppeh.rept.....a&link_type=abstract

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Physics

Dynamo Theory, Herbig-Haro Objects, Molecular Excitation, Plasma-Electromagnetic Interaction, Interstellar Gas, Plasma Heating, Plasma Sheaths, Plasma Waves, Stellar Winds

Scientific paper

The UV excess from highly ionized elements in the high-excitation Herbig-Haro objects is discussed. It is proposed that it can be explained if a sheath is formed in the object, with heating in excess of ordinary shock wave calculations. Such a sheath could be the result of dynamo interaction between a Herbig-Haro cloudlet and a magnetized stellar wind, with a transverse magnetic field of the order of 0.1 m Gauss.

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