Abstract
In this contribution, we present the STAGGERGRID, a collaborative project for the construction of a comprehensive grid of time-dependent, three-dimensional (3-D), hydrodynamic model atmospheres of solar- and late-type stars with different effective temperatures, surface gravities, and chemical compositions. We illustrate the main characteristics of these 3-D models and their effects on the predicted strengths, wavelength-shifts, and shapes of spectral lines, highlighting the differences with respect to calculations based on classical, one-dimensional, hydrostatic models, and discuss some of their possible applications to elemental abundance analysis of stellar spectra in the context of large observational surveys.
Originalsprog | Engelsk |
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Artikelnummer | 012003 |
Bogserie | Journal of Physics: Conference Series |
Vol/bind | 328 |
Udgave nummer | 1 |
Antal sider | 8 |
ISSN | 1742-6588 |
DOI | |
Status | Udgivet - 2011 |
Begivenhed | GREAT-ESF Workshop: Stellar Atmospheres in the Gaia Era - Vrije Universiteit Brussel, Bruxelles, Belgien Varighed: 23 jun. 2011 → 24 jun. 2011 |
Konference
Konference | GREAT-ESF Workshop |
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Lokation | Vrije Universiteit Brussel |
Land/Område | Belgien |
By | Bruxelles |
Periode | 23/06/2011 → 24/06/2011 |