Non-LTE model atmospheres are in the forefront of quantitative spectral analyses of early type stars. Yet, such models are barely used in large surveys or even for individual systems. The major reason for this is likely the extreme calculation requirements to construct such physically realistic models. To relieve this, we have developed a web-service for the spectral analysis program XTGRID, which is meant to be a handy interface to TLUSTY. Having the procedure available from a web browser makes spectral analyses a routine.
Radiative Signatures from the Cosmos
- Pub Date:
- July 2019
- Astrophysics - Solar and Stellar Astrophysics;
- Astrophysics - Instrumentation and Methods for Astrophysics
- 4 pages, 4 figures, to appear in "Radiative signatures from the Cosmos: A meeting in honor of Ivan Hubeny", 2018 October 23-26, Paris, France