Plasma processes in Herbig-Haro objects

Details Plasma processes in Herbig-Haro objects Plasma processes in Herbig-Haro objects

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.207..229a&link_type=abstract

In ESA Plasma Astrophys. p 229-233 (SEE N85-22270 12-90)

Astronomy and Astrophysics

Astrophysics

Cosmic Plasma, Herbig-Haro Objects, Stellar Spectra, Stellar Winds, Ultraviolet Spectra, Interstellar Magnetic Fields, Plasma Interactions, Plasma Sheaths, Shock Heating

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 mGauss.

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