Published December 1985
| Version v1
Journal article
On the broad Balmer profiles from car II and their possible origin as dust scattered lines from eta Carinae
Creators
- 1. Universidad Nacional Autonoma de Mexico, Mexico City. Inst. de Astronomia
- 2. Manchester Univ. (UK). Dept of Astronomy
Description
It is suggested that the high velocity components present in the Hα and Hβ lines over the entire face of the Car II region, in the Carinae nebula, could have their origin in the time varying emission from eta Carinae scattered by dust in the Car II region. (author)
Additional details
Publishing Information
- Journal Title
- Rev. Mex. Astron. Astrof.
- Journal Volume
- 11
- Journal Issue
- 2
- Series
- Rev. Mex. Astron. Astrof.
- Journal Page Range
- 71-72
- ISSN
- 0185-1101
- CODEN
- RMAAD
INIS
- Country of Publication
- Mexico
- Country of Input or Organization
- Mexico
- INIS RN
- 17042011
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BALMER LINES; COSMIC DUST; NEBULAE; STELLAR WINDS
- Descriptors DEC
- DUSTS; STELLAR ACTIVITY