activity
20062015
most citedStellar Diameters and Temperatures II. Main Sequence K & M Stars

593 citations · 3.7k across the 45 of their papers we have counts for

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Showing 2010Show all

7 papers · 1 filter

astro-ph.SR2010★ 2 cited

Fundamental Properties of Cool Stars with Interferometry

Tabetha S. Boyajian, K. von Braun, G. van Belle +11

We present measurements of fundamental astrophysical properties of nearby, low-mass, K- and M-dwarfs from our DISCOS survey (DIameterS of COol Stars). The principal goal of our stu…

astro-ph.SR2010★ 25 cited

The fundamental parameters of the roAp star Equulei

K. Perraut, I. Brandão, D. Mourard +18

Physical processes working in the stellar interiors as well as the evolution of stars depend on some fundamental stellar properties, such as mass, radius, luminosity, and chemical…

astro-ph.SR2010★ 10 cited

An investigation of the close environment of beta Cep with the VEGA/CHARA interferometer

N. Nardetto, D. Mourard, I. Tallon-Bosc +22

High-precision interferometric measurements of pulsating stars help to characterize their close environment. In 1974, a close companion was discovered around the pulsating star bet…

astro-ph.SR2010★ 37 cited

Multi-epoch Near-Infrared Interferometry of the Spatially Resolved Disk Around the Be Star Zeta Tau

G. H. Schaefer, D. R. Gies, J. D. Monnier +14

We present interferometric observations of the Be star Zeta Tau obtained using the MIRC beam combiner at the CHARA Array. We resolved the disk during four epochs in 2007-2009. We f…

astro-ph.SR2010★ 27 cited

Time, spatial, and spectral resolution of the Halpha line-formation region of Deneb and Rigel with the VEGA/CHARA interferometer

Olivier Chesneau, Luc Dessart, D. Mourard +22

BA-type supergiants are amongst the most optically-bright stars. They are observable in extragalactic environments, hence potential accurate distance indicators. Emission activity…

astro-ph.SR2010★ 19 cited

The H line forming region of AB Aur spatially resolved at sub-AU with the VEGA/CHARA spectro-interferometer

K. Perraut, M. Benisty, D. Mourard +19

A crucial issue in star formation is to understand the physical mechanism by which mass is accreted onto and ejected by a young star. The visible spectrometer VEGA on the CHARA arr…