Spectral variations among a sample of a stars in a limited range of effective temperature

Details Spectral variations among a sample of a stars in a limited range of effective temperature Spectral variations among a sample of a stars in a limited range of effective temperature

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apjs...39..429c&link_type=abstract

Astrophysical Journal Supplement Series, vol. 39, Mar. 1979, p. 429-438. NSF-supported research.

Astronomy and Astrophysics

Astrophysics

6

A Stars, Abundance, Line Spectra, Metallic Stars, Stellar Spectra, Anomalies, Astronomical Spectroscopy, Spectral Signatures

Scientific paper

We consider a number of sharp-lined spectra of stars within a narrow range of color and spectral type, having a variety of abundance peculiarities. A differential comparison of the spectra is made with the help of direct intensity tracings of selected wavelength regions. Complete wavelength measurements and identifications are given to illustrate specific abundance variations; several anomalies are pointed out, apparently for the first time.

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