Published February 1, 1980
| Version v1
Journal article
Very low-excitation Herbig-Haro objects
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
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 11553821
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BALMER LINES; ELECTRON DENSITY; ELECTRON TEMPERATURE; EMISSION SPECTRA; EXCITATION; HYDROMAGNETIC WAVES; INFRARED RADIATION; PROTOSTARS; SHOCK WAVES; SPECTROPHOTOMETRY
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ENERGY-LEVEL TRANSITIONS; RADIATIONS; SPECTRA