Asteroseismology of Stellar Populations in the Milky Way
The detection of radial and non-radial solar-like oscillations in thousands of G-K giants with CoRoT and Kepler is paving the road for detailed studies of stellar populations in the Galaxy. The available average seismic constraints allow largely model-independent determination of stellar radii and m...
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| Main Author: | |
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| Other Authors: | , , |
| Format: | Conference Paper |
| Language: | English |
| Published: |
Cham [u.a.]
Springer
2015
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| Series: | Astrophysics and Space Science Proceedings
39 SpringerLink Bücher |
| Volumes / Articles: | Show Volumes / Articles. |
| DOI: | 10.1007/978-3-319-10993-0 |
| Subjects: | |
| Online Access: | Verlag, Volltext: https://doi.org/10.1007/978-3-319-10993-0 Resolving-System, lizenzpflichtig, Volltext: http://dx.doi.org/10.1007/978-3-319-10993-0 Cover: https://swbplus.bsz-bw.de/bsz424912104cov.jpg |
| Author Notes: | edited by Andrea Miglio, Patrick Eggenberger, Léo Girardi, Josefina Montalbán |
Table of Contents:
- Ages of Stars: Methods and UncertaintiesSolar-Like Oscillating Stars as Standard Clocks and Rulers for Galactic Studies
- Uncertainties in Stellar Evolution Models: Convective Overshoot
- Effects of Rotation on Stellar Evolution and Asteroseismology of Red Giants
- Open Clusters: Probes of Galaxy Evolution and Bench Tests of Stellar Models
- Exploiting the Open Clusters in the Kepler and CoRoT Fields
- Photometric Stellar Parameters for Asteroseismology and Galactic Studies
- Spectroscopic Constraints for Low-Mass Asteroseismic Targets
- Preliminary Evaluation of the Kepler Input Catalog Extinction Model Using Stellar Temperatures
- The APOKASC Catalog
- The Red Giants in NGC 6633 as Seen with CoRoT, HARPS 30 and SOPHIE
- “Rapid-Fire” Spectroscopy of Kepler Solar-Like Oscillators
- New Observational Constraints to Milky Way ChemodynamicalModels
- The Expected Stellar Populations in the Kepler and CoRoT Fields
- Early Results from APOKASC
- The Metallicity Gradient of the Old Galactic Bulge Population
- 4MOST: 4m Multi Object Spectroscopic Telescope
- Mapping the Stellar Populations of the Milky Way with Gaia
- Uncertainties in Models of Stellar Structure and Evolution
- Photospheric Constraints, Current Uncertainties in Models of Stellar Atmospheres, and Spectroscopic Surveys.