Astronomy and Astrophysics – Astronomy
Scientific paper
May 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214p...9r&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, May 1, 1985, p. 9P-13P.
Astronomy and Astrophysics
Astronomy
21
Energy Sources, Herbig-Haro Objects, Infrared Spectra, Infrared Stars, Stellar Spectrophotometry, Ammonia, Near Infrared Radiation
Scientific paper
A possible source for the excitation energy of Herbig-Haro objects 1 and 2 has been detected at wavelengths of 1 - 4 μm. Its position coincides with a recent detection of a 6-cm radio continuum source and the centre of an NH3 torus orientated perpendicularly to the line joining H-H 1 and 2. Its infrared (1 - 200 μm) luminosity is approximately 10 L_sun;, consistent with a reddened (AV ≅ 12) T Tauri-type star. From upper limits in visual and near-infrared plates and from infrared photometry, a reddening law which resembles that of the Orion Belt and Sword regions has been calculated.
Rodriguez Luis F.
Roth Marcel
Tapia Mario
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