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Determining global parameters of the oscillations of solar-like stars
S. Mathur, R. A. Garcia, C. Regulo +7
Helioseismology has enabled us to better understand the solar interior, while also allowing us to better constrain solar models. But now is a tremendous epoch for asteroseismology…
HD172189: another step in furnishing one of the best laboratories known for asteroseismic studies
O. L. Creevey, K. Uytterhoeven, S. Martín-Ruiz +25
HD172189 is a spectroscopic eclipsing binary system with a rapidly-rotating pulsating delta Scuti component. It is also a member of the open cluster IC4756. These combined characte…
A Stellar Model-fitting Pipeline for Solar-like Oscillations
T. S. Metcalfe, O. L. Creevey, J. Christensen-Dalsgaard
Over the past two decades, helioseismology has revolutionized our understanding of the interior structure and dynamics of the Sun. Asteroseismology will soon place this knowledge i…
Radius determination of solar-type stars using asteroseismology: What to expect from the Kepler mission
D. Stello, W. J. Chaplin, H. Bruntt +22
For distant stars, as observed by the NASA Kepler satellite, parallax information is currently of fairly low quality and is not complete. This limits the precision with which the a…
A Stellar Model-fitting Pipeline for Asteroseismic Data from the Kepler Mission
T. S. Metcalfe, O. L. Creevey, J. Christensen-Dalsgaard
Over the past two decades, helioseismology has revolutionized our understanding of the interior structure and dynamics of the Sun. Asteroseismology will soon place this knowledge i…
A semi-automatic procedure for abundance determination of A- and F-type stars
S. Hekker, Y. Fremat, P. Lampens +4
A variety of physical processes leading to different types of pulsations and chemical compositions is observed among A- and F-type stars. To investigate the underlying mechanisms r…