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 Å - 10,000 Å using Non-LTE extensively line-blanketed atmosphere structures.

arXiv commentProceedings of the 10th meeting on hot subdwarfs and related objects. http://svo2.cab.inta-csic.es/theory/newov2/index.php?models=pacheco https://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/ApJS/256/41 http://specmodels.iag.usp.br/public_files/pacheco21/