Observed and computed UV spectral distribution of A and F stars

Details Observed and computed UV spectral distribution of A and F stars Observed and computed UV spectral distribution of A and F stars

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...114..170m&link_type=abstract

Astronomy and Astrophysics, vol. 114, no. 1, Oct. 1982, p. 170-176. Research supported by the Consiglio Nazionale delle Ricerch

Astronomy and Astrophysics

Astronomy

25

A Stars, F Stars, Spectral Energy Distribution, Stellar Spectra, Stellar Temperature, Ultraviolet Astronomy, Tables (Data), Visible Spectrum, Wavelengths

Scientific paper

An automatic and fast procedure was implemented to determine Te and log g from the comparison of the UV S 2/68 spectra with the Kurucz models. The method has been applied to all A and F stars with (B-V)0 greater than or equal to 0 and luminosity classes III, IV, IV-V, and V, included in the Ultraviolet Bright-Star Spectrophotometric Catalogue. From the analysis, it appears that the models match the observed fluxes fairly well and that the effective temperatures derived from the UV data agree with those derived from Stromgren photometric indices within 200 K.

Affiliated with

Also associated with

No associations

Rating

Observed and computed UV spectral distribution of A and F 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 Observed and computed UV spectral distribution of A and F stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observed and computed UV spectral distribution of A and F stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1028457