activity
19952004
collaborators

12 papers

astro-ph2004

Asteroseismology of Sun-like Stars - A Proposal

T. S. Metcalfe, T. M. Brown, J. Christensen-Dalsgaard

In the past decade, helioseismology has revolutionized our understanding of the interior structure of the Sun. In the next decade, asteroseismology will place this knowledge into c…

astro-ph2001

Rotation of the solar interior

J. Christensen-Dalsgaard, M. J. Thompson

Helioseismology has allowed us to infer the rotation in the greater part of the solar interior with high precision and resolution. The results show interesting conflicts with earli…

astro-ph2001

SOLA inversions for the core structure of solar-type stars

Sarbani Basu, J. Christensen-Dalsgaard, M. J. Thompson

The Subtractive Optimally Localized Averages (SOLA) method, developed and extensively used in helioseismology, is applied to artificial data to obtain measures of the sound speed i…

astro-ph2001

Asteroseismic Inference for Solar-Type Stars

M. J. P. F. G. Monteiro, J. Christensen-Dalsgaard, M. J. Thompson

The oscillation spectra of solar-type stars may in the not-too- distant future be used to constrain certain properties of the stars. The CD diagram of large versus small frequency…

astro-ph2000

The Effect of Diffusion on Pulsations of Stars on the Upper Main Sequence. delta Scuti and Metallic A Stars

S. Turcotte, J. Richer, G. Michaud +1

Recent dramatic improvements in the modeling of abundance evolution due to diffusion in A stars have been achieved with the help of monochromatic opacity tables from the OPAL group…

astro-ph1999

Amplitudes of stochastically excited oscillations in main-sequence stars

G. Houdek, N. J. Balmforth, J. Christensen-Dalsgaard +1

We present estimates of the amplitudes of intrinsically stable stochastically excited radial oscillations in stars near the main sequence. The amplitudes are determined by the bala…