Radii of some Ap, AM and A stars

Details Radii of some Ap, AM and A stars Radii of some Ap, AM and A stars

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..50..343b&link_type=abstract

Astrophysics and Space Science, vol. 50, no. 2, Aug. 1977, p. 343-348.

Astronomy and Astrophysics

Astrophysics

10

A Stars, Radii, Size Determination, Stellar Luminosity, Magnetic Stars, Main Sequence Stars, Stellar Evolution, Stellar Spectra

Scientific paper

Based on the observed energy curves of nine Ap stars, three Am stars, four normal A stars and one F0 V magnetic star, their radii have been estimated. Thence, the bolometric magnitudes have been obtained and a plot between the log of the electron temperature and bolometric magnitude of these stars shows that a majority of Ap and Am stars are a little above the zero-age main-sequence, suggesting that they are slightly more evolved as compared to the normal A stars. The bolometric corrections derived from the above bolometric magnitude are much closer to those computed by Mihalas (1966) than to the ones given by Davis and Webb (1970), the latter being about 0.1 m more negative than the former.

Affiliated with

Also associated with

No associations

Rating

Radii of some Ap, AM and A stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radii of some Ap, AM and A stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radii of some Ap, AM and A stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1880161