A discussion on the nature of the Herbig-Haro object no. 1 from its far UV spectrum

Details A discussion on the nature of the Herbig-Haro object no. 1 from its far UV spectrum A discussion on the nature of the Herbig-Haro object no. 1 from its far UV spectrum

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....83l...8o&link_type=abstract

Astronomy and Astrophysics, vol. 83, no. 3, Mar. 1980, p. L8, L9. Research supported by the Consiglio Nazionale delle Ricerche.

Astronomy and Astrophysics

Astronomy

44

Far Ultraviolet Radiation, Herbig-Haro Objects, Protostars, Ultraviolet Astronomy, Continuous Spectra, Emission Spectra, Line Spectra

Scientific paper

The first far UV observation of an Herbig-Haro object as shown a strong continuum and emission lines of C IV and C II. The intensities of the UV emission lines are not easily interpreted in the framework of the shock wave models which have been proposed for HH objects. The continuum increases toward the high frequencies and is not consistent with two photon emission from a hot gas.

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