The SAGA so far : Reading the history of the Galaxy with asteroseismology

Asteroseismology has the capability of delivering stellar properties which would otherwise be inaccessible, such as radii, masses and thus ages of stars. When this information is coupled with classical determinations of stellar parameters, such as metallicities, effective temperatures and angular diameters, powerful new diagnostics for stellar and Galactic studies can be obtained. The ongoing Strömgren survey for Asteroseismology and Galactic Archaeology (SAGA) is pursuing such a goal, by determining photometric stellar parameters for stars with seismic oscillations measured by the Kepler satellite. As the survey continues and expands in sample size, SAGA will provide an unprecedented opportunity to constrain theories of the evolution of the Milky Way disc.

Aguirre, Victor SilvaAarhus University (författare)
Serenelli, Aldo M.Autonomous University of Barcelona (författare)
Stello, DennisAarhus University,University of Sydney (författare)
Feltzing, SofiaLund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science(Swepub:lu)astr-sfe (författare)
Schlesinger, Katharine J.Australian National University (författare)
Australian National UniversityAarhus University (creator_code:org_t)

Av författaren/redakt...: Casagrande, Luca; Aguirre, Victor ...; Serenelli, Aldo ...; Stello, Dennis; Feltzing, Sofia; Schlesinger, Kat ...

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