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Analysis of Stellar Spectra with 3-D and NLTE Models

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Book cover Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars

Part of the book series: GeoPlanet: Earth and Planetary Sciences ((GEPS))

Abstract

Models of radiation transport in stellar atmospheres are the hinge of modern astrophysics. Our knowledge of stars, stellar populations, and galaxies is only as good as the theoretical models which are used for the interpretation of their observed spectra, photometric magnitudes, and spectral energy distributions. I describe recent advances in the field of stellar atmosphere modelling for late-type stars. Various aspects of radiation transport with 1-D hydrostatic, LTE, NLTE, and 3-D radiative-hydrodynamical models are briefly reviewed.

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Notes

  1. 1.

    Assuming that energy is transported by radiation only.

  2. 2.

    http://www.inspect-stars.net.

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Acknowledgments

Figure 1 reproduced by permission of the authors; the image was observed with the Swedish 1-m Solar Telescope. The SST is operated on the island of La Palma by the Institute for Solar Physics in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. The Institute for Solar Physics is a national research infrastructure under the Swedish Research Council. It is managed as an independent institute associated with Stockholm University through its Department of Astronomy. Figure 2: Asplund et al. A&A, 359, 729, 2000, reproduced with permission (c) ESO. Figures 3, 4 reproduced by permission of the AAS. Figure 8: Lind et al. A&A, 554, A96, 2013, reproduced with permission (c) ESO.

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Correspondence to Maria Bergemann .

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© 2014 Springer International Publishing Switzerland

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Bergemann, M. (2014). Analysis of Stellar Spectra with 3-D and NLTE Models. In: Niemczura, E., Smalley, B., Pych, W. (eds) Determination of Atmospheric Parameters of B-, A-, F- and G-Type Stars. GeoPlanet: Earth and Planetary Sciences. Springer, Cham. https://doi.org/10.1007/978-3-319-06956-2_17

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