The group of low-harmonic pulsating CP2 stars - HD 10088, a new candidate

Details The group of low-harmonic pulsating CP2 stars - HD 10088, a new candidate The group of low-harmonic pulsating CP2 stars - HD 10088, a new candidate

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...128..152w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 128, no. 1, Nov. 1983, p. 152-155. Research supported by the Max-Kade-Foundati

Astronomy and Astrophysics

Astrophysics

13

A Stars, Main Sequence Stars, Peculiar Stars, Stellar Oscillations, Chemical Composition, Dwarf Stars, Pulsars, Radiant Flux Density, Stellar Models, Stellar Spectrophotometry

Scientific paper

The CP2 star HD 10088 was found to be pulsating in the fundamental or
first overtone mode. Five CP2 stars are discussed as members of a group
of low-harmonic radially pulsating stars, a group which is clearly
distinct from the high overtone, non-radial oblique pulsators, a group
of eight stars established by Kurtz (1982).

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