Published December 15, 1988
| Version v1
Journal article
The spectrum of Canopus: Pt. 3
- 1. Canterbury Univ., Christchurch (New Zealand). Mt John University Observatory
Description
A careful search has been made for lines of elements heavier than the iron peak in the spectrum of Canopus, mainly using high signal-to-noise spectra in the near ultraviolet. The abundances of 21 heavy r-and s-process elements in Canopus have been determined from the equivalent widths of the lines identified. The results show that Canopus has an essentially solar composition for both r- and s-process heavy elements. Only for molybdenum and possibly niobium were deficiencies relative to the solar abundances found which are larger than can be explained by the estimated random errors of this analysis. (author)
Additional details
Additional titles
- Subtitle (English)
- Abundances of r- and s-process elements
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 235
- Journal Issue
- 4
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 1423-1438
- ISSN
- 0035-8711
- CODEN
- MNRAA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 20028045
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- CHEMICAL COMPOSITION; ELEMENT ABUNDANCE; ELEMENTS; EXPERIMENTAL DATA; LINE WIDTHS; MOLYBDENUM; NIOBIUM; R PROCESS; S PROCESS; SUPERGIANT STARS; ULTRAVIOLET SPECTRA; VISIBLE SPECTRA
- Descriptors DEC
- DATA; GIANT STARS; INFORMATION; METALS; NUMERICAL DATA; QUANTITY RATIO; SPECTRA; STAR EVOLUTION; STARS; TRANSITION ELEMENTS