Creating and Using Large Grids of Pre-calculated Model Atmospheres for Rapid Analysis of Stellar Spectra
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Publisher
Springer International Publishing
Link
http://link.springer.com/content/pdf/10.1007/978-3-030-38043-4_19
Reference22 articles.
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3. Castor, J.I., Abbott, D.C., Klein, R.I.: Radiation-driven winds in of stars. Astrophys. J. 195, 157–174 (1975)
4. Crowther, P.A., Hillier, D.J., Evans, C.J., Fullerton, A.W., De Marco, O., Willis, A.J.: Revised stellar temperatures of Magellanic cloud O supergiants from far ultraviolet spectroscopic explorer and Very Large Telescope UV- Visual Echelle Spectrograph spectroscopy. Astrophys. J. 579, 774–799 (2002)
5. Ekström, S., et al.: Grids of stellar models with rotation. I. Models from 0.8 to 120 M$$ \odot $$ at solar metallicity (Z = 0.014). A&A 537, A146 (2012)
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