Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aj....108.1432n&link_type=abstract
The Astronomical Journal, vol. 108, no. 4, p. 1432-1436
Astronomy and Astrophysics
Astronomy
17
Emission Spectra, Herbig-Haro Objects, Hydrogen, Infrared Astronomy, Infrared Imagery, Infrared Spectra, Molecular Excitation, Molecular Gases, Near Infrared Radiation, Ammonia, Astronomical Models, Astronomical Spectroscopy, Fluorescence, H Alpha Line, Infrared Spectroscopy, Infrared Telescopes, Interstellar Matter, Shock Waves, Sulfur
Scientific paper
We present a series of molecular hydrogen images of the Herbig-Haro 1-2 system in the 1-0 S(1) transition at 2.121 microns, with a spatial resolution of approximately 2 sec. The distribution of H2 is then compared with that of the excitation, given by the (S II) 6717+6731 to H-alpha line ratio. We find that most optical condensations in the HH 1-2 system, including the VLA 1 jet, have H2 counterparts. H2 emission is detected in most low excitation knots, as expected for low velocity shocks (50 km/s less than), but also in high excitation regions, like in HH 1F and HH 2A min. For these latter objects, the H2 emission could be due to the interaction of the preionizing flux, produced by 150-200 km/s shocks, with the surrounding interstellar matter, i.e., fluorescence. The lack fluorescent lines in the ultraviolet (UV), however, suggest a different mechanism. H2 is detected at the tip of the VLA 1 jet, where the knot morphology suggests the presence of a second bow shock. H2 is detected also SE of HH 2E and SW of HH 1F, in regions with known NH3 emission.
Garnavich Peter M.
Noriega-Crespo Alberto
No associations
LandOfFree
Molecular hydrogen and excitation in the HH 1-2 system does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Molecular hydrogen and excitation in the HH 1-2 system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Molecular hydrogen and excitation in the HH 1-2 system will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1069855