activity
20042026
most citedThe HARPS survey for southern extra-solar planets II. A 14 Earth-masses exoplanet around mu Arae

236 citations · 977 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2026

Dilution of accreted planetary matter in hot DA white dwarfs according to their mass

M. Deal, S. Vauclair, S. Charpinet +1

A large proportion of observed white dwarfs (WDs) show evidence of debris disks, remnants of the former planetary systems, and/or signatures of heavy elements in their atmospheres,…

astro-ph.SR2021★ 9 cited

New simulations of accreting DA white dwarfs: inferring accretion rates from the surface contamination

F. C. Wachlin, G. Vauclair, S. Vauclair +1

A non negligible fraction of white dwarf stars show the presence of heavy elements in their atmospheres. The most accepted explanation for this contamination is the accretion of ma…

astro-ph.SR2012★ 99 cited

The radius and mass of the close solar twin 18 Sco derived from asteroseismology and interferometry

M. Bazot, M. J. Ireland, D. Huber +28

The growing interest in solar twins is motivated by the possibility of comparing them directly to the Sun. To carry on this kind of analysis, we need to know their physical charact…

astro-ph.SR2012★ 30 cited

Estimating the p-mode frequencies of the solar twin 18 Sco

M. Bazot, T. L. Campante, W. J. Chaplin +17

Solar twins have been a focus of attention for more than a decade, because their structure is extremely close to that of the Sun. Today, thanks to high-precision spectrometers, it…

astro-ph.SR2011★ 104 cited

Accurate p-mode measurements of the G0V metal-rich CoRoT target HD 52265

J. Ballot, L. Gizon, R. Samadi +27

The star HD 52265 is a G0V metal-rich exoplanet-host star observed in the seismology field of the CoRoT space telescope from November 2008 to March 2009. The satellite collected 11…

astro-ph2008

CoRoT measures solar-like oscillations and granulation in stars hotter than the Sun

E. Michel, A. Baglin, M. Auvergne +2

Oscillations of the Sun have been used to understand its interior structure. The extension of similar studies to more distant stars has raised many difficulties despite the strong…