J/A+AS/110/553 Teff for B, A and F main sequence stars (Sokolov, 1995)
The determination of Teff of B, A and F main sequence stars from
the continuum between 3200 A and 3600 A.
SOKOLOV N.A.
<Astron. Astrophys. Suppl. Ser. 110, 553 (1995)>
=1995A&AS..110..553S 1995A&AS..110..553S (SIMBAD/NED Reference)
ADC_Keywords: Spectrophotometry; Ultraviolet; Stars, B-type; Stars, A-type;
Stars, F-type; Effective temperatures
Keywords: stars: atmospheres - stars: early-type -
stars: fundamental parameters
Description:
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.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table3 49 235 Balmer jumps, effective temperatures and
their errors for the 235 program stars.
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Byte-by-byte Description of file: table3
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Bytes Format Units Label Explanations
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1- 4 I4 --- HR Number in the Bright Star Catalogue
6- 11 I6 --- HD Number in the Henry Draper Catalogue
14- 24 A11 --- Sp Spectral Type
27- 31 F5.2 mag E(B-V) Colour excess
34- 38 F5.3 --- D Balmer jump (in dex)
40- 44 I5 K Teff Temperature
46- 49 I4 K e_Teff rms uncertainty on temperature
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(End) Patricia Bauer [CDS] 06-Jan-1995