Spectrophotometry of B, A, and F stars. III.
Abstract
Optical region energy distributions of 13 bright normal B, A, and F stars consistent with the Hayes-Latham calibration of Vega are presented. These scans contain more wavelength values than those given in previous papers in this series. The procedure of synthesizing u-b and b-y values from spectrophotometry is improved. Effective temperatures are found using the empirical calibration of Code and his colleagues and the fully line-blanketed solar composition model atmospheres of Kurucz.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- March 1983
- DOI:
- 10.1086/160819
- Bibcode:
- 1983ApJ...266..732A
- Keywords:
-
- A Stars;
- B Stars;
- Early Stars;
- F Stars;
- Stellar Spectrophotometry;
- Stellar Temperature;
- Solar Atmosphere;
- Spectral Energy Distribution;
- Stellar Atmospheres;
- Stellar Spectra;
- Ultraviolet Photometry;
- Astronomy