H2 emission from Herbig-Haro objects

Details H2 emission from Herbig-Haro objects H2 emission from Herbig-Haro objects

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...241..728e&link_type=abstract

Astrophysical Journal, Part 1, vol. 241, Oct. 15, 1980, p. 728-735.

Astronomy and Astrophysics

Astrophysics

89

Emission Spectra, Herbig-Haro Objects, Hydrogen, Infrared Spectra, Stellar Spectra, Radial Velocity, Radiant Flux Density, Shock Heating, Spectral Line Width

Scientific paper

Molecular hydrogen emission lines have been detected in six Herbig-Haro objects. The line intensities suggest that the H2 emission arises in a moderate-density, shock-heated gas, consistent with evidence for a similar origin of the visible emission-line spectra in Herbig-Haro objects. Indirect arguments indicate that the typical H2 line widths are less than 70 km/sec and that typical heliocentric radial velocities are no more than 30 km/sec in magnitude.

Affiliated with

Also associated with

No associations

Rating

H2 emission from Herbig-Haro objects 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 H2 emission from Herbig-Haro objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and H2 emission from Herbig-Haro objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-947674