Published April 26, 2019
| Submitted
Report
Open
Astro2020 Science White Paper: Stellar Physics and Galactic Archeology using Asteroseismology in the 2020's
- Creators
-
Huber, Daniel
- Basu, Sarbani
- Beck, Paul
- Bedding, Timothy R.
- Buzasi, Derek
- Cantiello, Matteo
- Chaplin, William J.
- Christiansen, Jessie L.
- Cunha, Katia
- Egeland, Ricky
-
Fuller, Jim
- Garcia, Rafael A.
- Gies, Douglas R.
- Guzik, Joyce
- Hekker, Saskia
- Hermes, J. J.
- Jackiewicz, Jason
- Johnson, Jennifer
- Kawaler, Steve
- Metcalfe, Travis
- Mosser, Benoit
- Ness, Melissa
- Pinsonneault, Marc
- Piro, Anthony L.
- Silva Aguirre, Victor
- Soderblom, David
- Stassun, Keivan
- Tayar, Jamie
-
ten Brummelaar, Theo
- Roettenbacher, Rachael
- Sobeck, Jennifer
- Trampedach, Regner
- van Belle, Gerard
- van Saders, Jennifer
- Stello, Dennis
Abstract
Asteroseismology is the only observational tool in astronomy that can probe the interiors of stars, and is a benchmark method for deriving fundamental properties of stars and exoplanets. Over the coming decade, space-based and ground-based observations will provide a several order of magnitude increase of solar-like oscillators, as well as a dramatic increase in the number and quality of classical pulsator observations, providing unprecedented possibilities to study stellar physics and galactic stellar populations. In this white paper, we describe key science questions and necessary facilities to continue the asteroseismology revolution into the 2020's.
Attached Files
Submitted - 1903.08188.pdf
Files
1903.08188.pdf
Files
(1.5 MB)
| Name | Size | Download all |
|---|---|---|
|
md5:8dcf837d9cc8e343e32d2a87daa2d332
|
1.5 MB | Preview Download |
Additional details
- Eprint ID
- 95008
- Resolver ID
- CaltechAUTHORS:20190426-083226413
- Created
-
2019-04-26Created from EPrint's datestamp field
- Updated
-
2023-06-02Created from EPrint's last_modified field
- Caltech groups
- Astronomy Department
- Series Name
- Astro2020 Science White Paper