A Grid of Synthetic Spectra for Subdwarfs: Non-LTE Line-blanketed Atmosphere Models

A new grid of detailed atmosphere model spectra for hot and moderately cool subdwarf stars is presented. High-resolution spectra and synthetic photometry are calculated in the range from 1000{\AA} to 10,000{\AA} using Non-LTE fully line-blanketed atmosphere structures. Our grid covers eight temperatures within 10,000

Keywords:

• Photometry (optics)
• Atmosphere
• Line (formation)
• Spectral line
• Astrophysics
• Stars
• Galactic halo
• Physics
• Subdwarf
• Metallicity

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