Zobrazeno 1 - 4
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pro vyhledávání: '"Maria Bergemann"'
Autor:
Thomas Nordlander, Maria Bergemann
Publikováno v:
Determination of Atmospheric Parameters of B-, A-, F-and G-Type Stars ISBN: 9783319069555
The interpretation of observed spectra of stars in terms of fundamental stellar properties is a key problem in astrophysics. For FGK-type stars, the radiative transfer models are often computed using the assumption of local thermodynamic equilibrium
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d8e3ae5e05f01f971d473085acf91687
https://doi.org/10.1007/978-3-319-06956-2_16
https://doi.org/10.1007/978-3-319-06956-2_16
Autor:
Maria Bergemann
Publikováno v:
Determination of Atmospheric Parameters of B-, A-, F-and G-Type Stars ISBN: 9783319069555
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 spe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::24f7194b86ecdc6ab38318d1b029d89a
https://doi.org/10.1007/978-3-319-06956-2_17
https://doi.org/10.1007/978-3-319-06956-2_17
Autor:
Aldo Serenelli, Maria Bergemann
Publikováno v:
Determination of Atmospheric Parameters of B-, A-, F-and G-Type Stars ISBN: 9783319069555
The chemical composition of the Sun is among the most important quantities in astrophysics. Solar abundances are needed for modelling stellar atmospheres, stellar structure and evolution, population synthesis, and galaxies as a whole. The solar abund
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b9be1839893bce7039ef7b25d6eb4648
https://doi.org/10.1007/978-3-319-06956-2_21
https://doi.org/10.1007/978-3-319-06956-2_21
Publikováno v:
Determination of Atmospheric Parameters of B-, A-, F-and G-Type Stars ISBN: 9783319069555
Cool red giants and supergiants are among the most complex and fascinating stars in the Universe. They are bright and large, and thus can be observed to enormous distances allowing us to study the properties of their host galaxies, such as dynamics a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0bb07ed5f4b54ad119a63115710ff6b5
https://doi.org/10.1007/978-3-319-06956-2_19
https://doi.org/10.1007/978-3-319-06956-2_19