Volume 413, Number 1, January I 2004
|Page(s)||323 - 327|
|Section||Stellar structure and evolution|
|Published online||17 December 2003|
Physical parameters of helium-rich subdwarf B stars from spectral energy distributions*
Armagh Observatory, College Hill, Armagh BT61 9DG., N. Ireland, UK
Corresponding author: A. Ahmad, firstname.lastname@example.org
Accepted: 2 October 2003
We present effective temperatures and angular radii for eleven helium-rich subdwarf B stars. These are measured using spectral energy distributions from archival IUE spectra and existing optical and infrared photometry. The data have been analysed using a grid of high-gravity helium-rich LTE model atmospheres and a -minimization procedure. The parameters derived here allow for independent verification of the parameters derived from the analysis of optical spectra.
Key words: stars: chemically peculiar / stars: early-type / subdwarfs / stars: atmospheres / stars: fundamental parameters
© ESO, 2004
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