Bibcode
Malagnini, M. L.; Faraggiana, R.; Morossi, C.; Crivellari, L.
Referencia bibliográfica
Astronomy and Astrophysics, vol. 114, no. 1, Oct. 1982, p. 170-176. Research supported by the Consiglio Nazionale delle Ricerche.
Fecha de publicación:
10
1982
Revista
Número de citas
27
Número de citas referidas
24
Descripción
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.