On the radii of AP and AM stars

Details On the radii of AP and AM stars On the radii of AP and AM stars

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..89..341b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 89, no. 2, Jan. 1983, p. 341-344.

Astronomy and Astrophysics

Astrophysics

3

A Stars, Magnetic Stars, Peculiar Stars, Radii, S Stars, Stellar Magnitude

Scientific paper

The radii of several Ap and Am stars have been compared with those of the normal A stars of the main sequence. Though the brighter Ap stars have a little larger radii than the main sequence stars, they may not be much different from those of the slightly evolved normal A stars. The Am stars have radii with which they appear to be merging with those of cooler A stars of the main sequence. The Ap stars have radii predominantly in the range of 1.8 to 3.4 solar radii, while the Am stars are mainly concentrated between 1.8 and 2.2 solar radii.

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