Asteroseismology of Stellar Populations in the Milky Way [E-Book] / edited by Andrea Miglio, Patrick Eggenberger, Léo Girardi, Josefina Montalbán.
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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Full text |
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Personal Name(s): | Eggenberger, Patrick, editor |
Girardi, Léo, editor / Miglio, Andrea, editor / Montalbán, Josefina, editor | |
Edition: |
1st ed. 2015. |
Imprint: |
Cham :
Springer,
2015
|
Physical Description: |
XIII, 185 pages 49 illustrations, 3 illustrations in color (online resource) |
Note: |
englisch |
ISBN: |
9783319109930 |
DOI: |
10.1007/978-3-319-10993-0 |
Series Title: |
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Astrophysics and Space Science Proceedings ;
39 |
- Ages of Stars: Methods and Uncertainties
- Solar-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.