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Asteroseismology for Galactic archaeology: bridging two fields

Published online by Cambridge University Press:  27 October 2016

Luca Casagrande ,
Victor Silva Aguirre  and
Aldo M. Serenelli
Luca Casagrande
Affiliation:
Research School of Astronomy & Astrophysics, Mount Stromlo Observatory The Australian National University, ACT 2611, Australia
Victor Silva Aguirre
Affiliation:
Stellar Astrophysics Centre, Department of Physics and Astronomy Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
Aldo M. Serenelli
Affiliation:
Instituto de Ciencias del Espacio (ICE-CSIC/IEEC) Campus UAB Carrer de Can Magrans, s/n 08193 Cerdanyola del Valls, Spainhttp://www.mso.anu.edu.au/saga
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Abstract

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Asteroseismology has the capability of precisely determining stellar properties that would otherwise be inaccessible, such as radii, masses, and thus ages of field stars. When coupling this information with classical determinations of stellar parameters, such as metallicities, effective temperatures, and angular diameters, powerful new diagnostics for Galactic studies can be obtained. An overview of the ongoing Strömgren survey for Asteroseismology and Galactic Archaeology (SAGA) is presented, along with recent results using asteroseismology to investigate the vertical age structure of the Milky Way disc.

Keywords

Galaxy: stellar contentGalaxy: discGalaxy: evolutionstars: fundamental parametersstars: oscillationssurveystechniques: photometric
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 680 - 685
Copyright
Copyright © International Astronomical Union 2016 

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