Very low-excitation Herbig-Haro objects

Details Very low-excitation Herbig-Haro objects Very low-excitation Herbig-Haro objects

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235l.137b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 235, Feb. 1, 1980, p. L137-L141.

Astronomy and Astrophysics

Astrophysics

31

Herbig-Haro Objects, Line Spectra, Shock Waves, Stellar Spectrophotometry, Emission Spectra, Forbidden Bands, Stellar Envelopes

Scientific paper

Spectrophotometric observations show that H-H 7 and H-H 11 belong to a class of very low-excitation Herbig-Haro objects of which H-H 47 has been the only known example. Typical properties include line flux ratios which are considerably larger than 1, very strong (O I) and (C I) lines, as well as relatively faint (O II) lines. So far no shock-wave models are available for these low-excitation objects. H-H 7 and H-H 11 have electron densities which are lower by about one order of magnitude, and electron temperatures which are slightly lower than those for high-excitation objects.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1620594