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19932026
most citedThe Gaia mission

7.1k citations

Showing 2009Show all

88 papers · 1 filter

astro-ph.SR2009★ 480 cited

Kepler Asteroseismology Program: Introduction and First Results

Ronald L. Gilliland, T. M. Brown, J. Christensen-Dalsgaard +32

Asteroseismology involves probing the interiors of stars and quantifying their global properties, such as radius and age, through observationsof normal modes of oscillation. The te…

astro-ph.EP2009★ 38 cited

A substellar component orbiting the F-star 30 Ari B

E. W. Guenther, M. Hartmann, M. Esposito +3

CONTEXT: Most current radial velocity planet search programs have concentrated on stars of one solar mass. Our knowledge on the frequency of giant planets and brown dwarf companion…

astro-ph.SR2009★ 10 cited

Asteroseismic modelling of the solar-like star Hydri

G. Doğan, I. M. Brandão, T. R. Bedding +3

We present the results of modelling the subgiant star Hydri using the seismic observational constraints. We have computed several grids of stellar evolutionary tracks using Aar…

astro-ph.SR2009★ 26 cited

The radius and effective temperature of the binary Ap star beta CrB from CHARA/FLUOR and VLT/NACO observations

H. Bruntt, P. Kervella, A. Merand +14

The prospects for using asteroseismology of rapidly oscillating Ap (roAp) stars are hampered by the large uncertainty in fundamental stellar parameters. Results in the literature f…

astro-ph.EP2009★ 28 cited

The HARPS search for southern extra-solar planets. XX. Planets around the active star BD-08:2823

G. Hebrard, S. Udry, G. Lo Curto +13

We report the detection of a planetary system around BD-08:2823, that includes at least one Uranus-mass planet and one Saturn-mass planet. This discovery serendipitously originates…

astro-ph.SR2009★ 1 cited

Observational signatures for depletion in the Spite plateau: solving the cosmological Li discrepancy?

J. Melendez, L. Casagrande, I. Ramirez +2

We present Li abundances for 73 stars in the metallicity range -3.5 < [Fe/H] < -1.0 using improved IRFM temperatures (Casagrande et al. 2010) with precise E(B-V) values obtained mo…