The exciting star of Herbig-Haro object 1

Details The exciting star of Herbig-Haro object 1 The exciting star of Herbig-Haro object 1

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...233l..77c&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 233, Oct. 15, 1979, p. L77-L80. Research supported by the University

Astronomy and Astrophysics

Astronomy

73

Herbig-Haro Objects, Infrared Stars, Stellar Spectra, T Tauri Stars, Emission Spectra, Energy Distribution, Infrared Astronomy, Line Spectra

Scientific paper

A star close to HH 1 is a bright infrared source. Its optical spectrum shows it to be a highly obscured T Tauri star. It is argued that this is the source of excitation of HH 1, and perhaps also of HH 2. The likely mass-loss rate is of the order of 10 to the -8th to 10 to the -7th solar mass/yr, depending on the geometry of outflow from the star. Another infrared object may contribute to the excitation of HH 2.

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