Detection of H2 emission in Herbig-Haro object No. 101

Details Detection of H2 emission in Herbig-Haro object No. 101 Detection of H2 emission in Herbig-Haro object No. 101

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203..785b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 203, May 1983, p. 785-789. Research supported by the Ox

Astronomy and Astrophysics

Astronomy

11

Astronomical Spectroscopy, Emission Spectra, H Lines, Herbig-Haro Objects, Broadband, Hydrogen, Molecular Gases, Spectral Energy Distribution, Stellar Models

Scientific paper

H2 emission in the spectrum of HH 101 has been detected. The
linestrength of the v = 1-0 S(1) line at 2.12 microns is (4.2 + or -
0.6) x 10 to the -17th W/sq m and indicates that a shock with a velocity
of about 14 km/s is moving into a cloud of density about 1000 per cu cm
if Schwartz's model for Herbig-Haro objects is valid.

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