Published May 1980
| Version v1
Journal article
On the emission-line intensities and light-curve characteristics of Orion-population stars
Creators
- 1. Monterey Inst. for Research in Astronomy, Carmel Valley, CA (USA)
Description
The Orion-population stars listed in the Herbig-Rao catalogue show a strong correlation between Parenago light-curve classification and emission-line intensities in a sense different from that expected from the behaviour of individual stars. In addition, the range in brightness variability of these stars appears to be independent of emission-line strength and light-curve classification. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 191
- Journal Issue
- 2
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 321-324
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 11539892
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BRIGHTNESS; CORRELATIONS; EMISSION SPECTRA; STARS; STATISTICAL MODELS; VARIATIONS
- Descriptors DEC
- MATHEMATICAL MODELS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; SPECTRA