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