On the infrared emission of the exciting star of the Herbig-Haro objects 1 and 2

Details On the infrared emission of the exciting star of the Herbig-Haro objects 1 and 2 On the infrared emission of the exciting star of the Herbig-Haro objects 1 and 2

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.224..587t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 224, Feb. 1, 1987, p. 587-593.

Astronomy and Astrophysics

Astronomy

7

Herbig-Haro Objects, Infrared Stars, Stellar Envelopes, T Tauri Stars, Emission Spectra, Interstellar Extinction

Scientific paper

Further evidence is presented indicating that the infrared emission at λ > 3 μm, spatially coincident with the VLA source located midway between the Herbig-Haro objects 1 and 2, comes from warm circumstellar dust around the star most probably responsible for the excitation of these Herbig-Haro objects. The nearby extended emission dominating at shorter wavelengths comes from scattered stellar light, the shocked ionized nebulosity, or both. The visual extinction in the direction of the central star is 23 ⪉ AV ⪉ 63.

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