The determination of Teff of B, A and F main sequence stars from the continuum between 3200 A and 3600 A. J/A+AS/110/553 J/A+AS/110/553 Teff for B, A and F main sequence stars The determination of Teff of B, A and F main sequence stars from the continuum between 3200 A and 3600 A. N A Sokolov Astron. Astrophys. Suppl. Ser. 110 553 1995 1995A&AS..110..553S stars: atmospheres stars: early-type stars: fundamental parameters A method of determination of the effective temperature of B, A and F main sequence stars is proposed, using the slope of the continuum between 3200A and 3600A. We have determined the Balmer jump and the effective temperatures for 235 main sequence stars.
Balmer jumps, effective temperatures and their errors for the 235 program stars. HR Number in the Bright Star Catalogue --- HD Number in the Henry Draper Catalogue --- Sp Spectral Type --- E(B-V) Colour excess mag D Balmer jump (in dex) --- Teff Temperature K e_Teff rms uncertainty on temperature K Patricia Bauer CDS 1995Jan06 J_A+AS_110_553.xml