An analysis of HD 43819 by wavelength-coincidence statistics

Details An analysis of HD 43819 by wavelength-coincidence statistics An analysis of HD 43819 by wavelength-coincidence statistics

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pasp...99..623p&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 99, July 1987, p. 623-628.

Statistics

6

Line Spectra, Peculiar Stars, Spectrum Analysis, Statistical Analysis, Stellar Composition, Wavelengths, Metallicity, Molybdenum, Neodymium

Scientific paper

An element identification study has been performed on the sharp-lined Si star HD 43819 using the method of wavelength-coincidence statistics (WCS). The results are compared to a study by Adelman (1985) who used traditional methods. The data generally confirm the previous investigation but also provide evidence to support the identifications of Dy III, Gd II, Nd III, and Mo II.

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