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Paper: Synthetic Spectra for O and B Type Subdwarf Stars
Volume: 481, 6th Meeting on Hot Subdwarf Stars and Related Objects
Page: 95
Authors: Nemeth, P.; Østensen, R.; Tremblay, P.; Hubeny, I.
Abstract: We present a grid of optical (3200–7200 Å) synthetic spectra calculated with TLUSTY/SYNSPEC. The new NLTE model atmospheres include the most recent hydrogen Stark broadening profiles; were calculated in opacity sampling and limited to pure H/He composition. The grid covers the observed parameter space of (He-)sdB and (He-)sdO stars, therefore it is suitable for the homogeneous spectral analyses of such evolved stars.
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