activity
20052024
most citedFirst Results from the CHARA Array. II. A Description of the Instrument

517 citations · 2.6k across the 56 of their papers we have counts for

collaborators
Showing 2017Show all

6 papers · 1 filter

astro-ph.SR2017★ 37 cited

Contemporaneous Imaging Comparisons of the Spotted Giant Geminorum Using Interferometric, Spectroscopic, and Photometric Data

Rachael M. Roettenbacher, John D. Monnier, Heidi Korhonen +8

Nearby, active stars with relatively rapid rotation and large starspot structures offer the opportunity to compare interferometric, spectroscopic, and photometric imaging technique…

astro-ph.SR2017★ 104 cited

No Sun-like dynamo on the active star Andromedae from starspot asymmetry

Rachael M. Roettenbacher, John D. Monnier, Heidi Korhonen +12

Sunspots are cool areas caused by strong surface magnetic fields inhibiting convection. Moreover, strong magnetic fields can alter the average atmospheric structure, degrading our…

astro-ph.EP2017★ 8 cited

The peculiar fast-rotating star 51 Oph probed by VEGA/CHARA

Narges Jamialahmadi, Philippe Berio, Anthony Meilland +15

Stellar rotation is a key in our understanding of both mass-loss and evolution of intermediate and massive stars. It can lead to anisotropic mass-loss in the form of radiative wind…

astro-ph.IM2017★ 5 cited

Visibility Estimation for the CHARA/JouFLU Exozodi Survey

Paul D. Nunez, Theo ten Brummelaar, Bertrand Mennesson +1

We discuss the estimation of the interferometric visibility (fringe contrast) for the exozodi survey conducted at the CHARA array with the JouFLU beam combiner. We investigate the…

astro-ph.SR2017★ 14 cited

A near-infrared interferometric survey of debris-disk stars. VI. Extending the exozodiacal light survey with CHARA/JouFLU

Paul D. Nunez, N. J. Scott, B. Mennesson +11

We report the results of high-angular-resolution observations that search for exozodiacal light in a sample of main sequence stars and sub-giants. Using the "jouvence" of the fiber…

astro-ph.SR2017★ 5 cited

Science cases for a visible interferometer

Philippe Stee, France Allard, Myriam Benisty +54

High spatial resolution is the key for the understanding various astrophysical phenomena. But even with the future E-ELT, single dish instruments are limited to a spatial resolutio…