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20012019
most citedFundamental Properties of Stars using Asteroseismology from Kepler & CoRoT and Interferometry from the CHARA Array

260 citations · 1.4k across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.EP2019★ 10 cited

Building protoplanetary disks from the molecular cloud: redefining the disk timeline

Kevin Baillié, Joao Marques, Laurent Piau

We study the formation of the protoplanetary disk by the collapse of a primordial molecular cloud, and how its evolution leads to the selection of specific types of planets. We use…

astro-ph.SR2013★ 40 cited

Models of solar surface dynamics: impact on eigenfrequencies and radius

Laurent Piau, Remo Collet, Robert F. Stein +3

We study the effects of different descriptions of the solar surface convection on the eigenfrequencies of p-modes. 1-D evolution calculations of the whole Sun and 3-D hydrodynamic…

astro-ph.SR2012★ 260 cited

Fundamental Properties of Stars using Asteroseismology from Kepler & CoRoT and Interferometry from the CHARA Array

D. Huber, M. J. Ireland, T. R. Bedding +37

We present results of a long-baseline interferometry campaign using the PAVO beam combiner at the CHARA Array to measure the angular sizes of five main-sequence stars, one subgiant…

astro-ph.SR2012★ 200 cited

A uniform asteroseismic analysis of 22 solar-type stars observed by Kepler

S. Mathur, T. S. Metcalfe, M. Woitaszek +39

Asteroseismology with the Kepler space telescope is providing not only an improved characterization of exoplanets and their host stars, but also a new window on stellar structure a…

astro-ph.SR2012★ 32 cited

Comparison of Fe and Ni opacity calculations for a better understanding of pulsating stellar envelopes

D. Gilles, S. Turck-Chièze, G. Loisel +19

Opacity is an important ingredient of the evolution of stars. The calculation of opacity coefficients is complicated by the fact that the plasma contains partially ionized heavy io…

astro-ph.SR2012★ 28 cited

On plasma radiative properties in stellar conditions

S. Turck-Chièze, F. Delahaye, D. Gilles +2

The knowledge of stellar evolution is evolving quickly thanks to an increased number of opportunities to scrutinize the stellar internal plasma properties by stellar seismology and…