Published November 1982
| Version v1
Journal article
On the nature of the stellar population in the nucleus of the Sd galaxy NGC 7793
- 1. Royal Greenwich Observatory, Hailsham (UK)
- 2. University Coll. of South Wales and Monmouthshire, Cardiff (UK)
- 3. Cerro Tololo Inter-American Observatory, La Serena (Chile)
Description
Profiles and equivalent widths of hydrogen, Ca+ and some other lines imply that the blue-violet spectrum of the nucleus of this late-type spiral is dominated by A or early F stars near the main sequence and not by a mixture of globular cluster-like populations. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 201
- Journal Issue
- 2
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 49P-55P
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 14777832
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- EXPERIMENTAL DATA; GALAXIES; GALAXY NUCLEI; LINE WIDTHS; SPIRAL CONFIGURATION; STAR CLUSTERS; VISIBLE SPECTRA
- Descriptors DEC
- CONFIGURATION; DATA; INFORMATION; NUMERICAL DATA; SPECTRA