A grid of Non-LTE line-blanketed atmosphere structures and synthetic spectra for subdwarfs
Abstract
We present an update of the grid of detailed atmosphere models and homogeneous synthetic spectra for hot, high-gravity subdwarf stars. High-resolution spectra and synthetic photometry were calculated in the wavelength range 1,000 A - 10,000 A using Non-LTE extensively line-blanketed atmosphere structures.
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