activity
19972017
most citedThe diameters of Alpha Centauri A and B - A comparison of the asteroseismic and VINCI/VLTI views

160 citations · 1.3k across the 23 of their papers we have counts for

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19 papers · 1 filter

astro-ph2008★ 3 cited

The seismology programme of CoRoT

E. Michel, A. Baglin, M. Auvergne +1

We introduce the main lines and specificities of the CoRoT Seismology Core Programme. The development and consolidation of this programme has been made in the framework of the CoRo…

astro-ph2008★ 158 cited

A multi-site campaign to measure solar-like oscillations in Procyon. I. Observations, Data Reduction and Slow Variations

Torben Arentoft, Hans Kjeldsen, Timothy R. Bedding +45

We have carried out a multi-site campaign to measure oscillations in the F5 star Procyon A. We obtained high-precision velocity observations over more than three weeks with eleven…

astro-ph2008★ 44 cited

Update on g-mode research

R. A. Garcia, A. Jimenez, S. Mathur +6

Since the beginning of this century we have attended a blooming of the gravity-mode research thanks to the unprecedented quality of the data available, either from space with SoHO,…

astro-ph2007★ 22 cited

Asteroseismology of Procyon with SOPHIE

B. Mosser, F. Bouchy, M. Martic

This paper reports a 9-night asteroseismic observation program conducted in January 2007 with the new spectrometer Sophie at the OHP 193-cm telescope, on the F5 IV-V target Procyon…

astro-ph2007★ 38 cited

Inter-comparison of the g-, f- and p-modes calculated using different oscillation codes for a given stellar model

A. Moya, J. Christensen-Dalsgaard, S. Charpinet +9

In order to make astroseismology a powerful tool to explore stellar interiors, different numerical codes should give the same oscillation frequencies for the same input physics. Th…

astro-ph2007★ 3 cited

Oscillations in Procyon A: First results from a multi-site campaign

S. Hekker, T. Arentoft, H. Kjeldsen +45

Procyon A is a bright F5IV star in a binary system. Although the distance, mass and angular diameter of this star are all known with high precision, the exact evolutionary state is…