Published February 1, 1980 | Version v1
Journal article

Very low-excitation Herbig-Haro objects

  • 1. Astronomy Department, University of Washington

Description

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 [N I] (lambda5198+lambda5200)/Hβ and [S II] lambda/6717/Hα, which are both 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 like H-H 1 and H-H 2. H-H 11 has a filling factor of about 1, much higher than other H-H objects

Additional details

Publishing Information

Journal Title
Astrophys. J., Lett. Ed.
Journal Volume
235
Journal Issue
3
Series
Astrophys. J., Lett. Ed.
Journal Page Range
L137-L141