Metallicism and pulsation - The marginal metallic line stars

Details Metallicism and pulsation - The marginal metallic line stars Metallicism and pulsation - The marginal metallic line stars

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...221..869k&link_type=abstract

Astrophysical Journal, Part 1, vol. 221, May 1, 1978, p. 869-880.

Astronomy and Astrophysics

Astrophysics

44

A Stars, Astronomical Photometry, Line Spectra, Metallic Stars, Stellar Spectra, Variable Stars, Data Acquisition, Hertzsprung-Russell Diagram, Light Curve, Stellar Spectrophotometry

Scientific paper

Evidence is presented that HR 4594 and HR 8210 are pulsating marginal Am stars. It is suggested that (1) classical Am stars do not pulsate, (2) evolved Am stars may pulsate, and (3) marginal Am stars may pulsate. It is further suggested that, within the Am domain, temperature, age, rotation, and pulsation are sufficient to determine whether a star will be Am, marginal Am, or spectrally normal.

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