Bolometric corrections for peculiar B-type stars

Details Bolometric corrections for peculiar B-type stars Bolometric corrections for peculiar B-type stars

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...139..161l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 139, no. 1, Oct. 1984, p. 161-170. Sponsorship: Research suppported by the Swi

Astronomy and Astrophysics

Astrophysics

35

B Stars, Bolometers, Error Analysis, Peculiar Stars, Stellar Spectrophotometry, Ultraviolet Spectra, Interstellar Extinction, Iue, Main Sequence Stars, Paschen Series, Radiant Flux Density

Scientific paper

Semi-empirical bolometric corrections are estimated for 25 peculiar stars and 13 comparison stars from IUE low dispersion spectrum and from theoretical fluxes best fitting the Geneva colour indices. When corrected for reddening, the relation BC vs. (B2-G)0 for main-sequence stars matches fairly well the theoretical relation computed by Kurucz. The difference on BC between a peculiar star and a comparison star with the same Paschen slope is less than 0.3 mag. A quantitative estimation of the UV deficiency of CP stars is also given.

Affiliated with

Also associated with

No associations

Rating

Bolometric corrections for peculiar B-type 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 Bolometric corrections for peculiar B-type stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bolometric corrections for peculiar B-type stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1226309