activity
20072021
most citedNo Sun-like dynamo on the active star Andromedae from starspot asymmetry

104 citations · 372 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2021★ 24 cited

A near-infrared interferometric survey of debris-disk stars. VII. The hot/warm dust connection

O. Absil, L. Marion, S. Ertel +10

(abridged) Context. The origin of hot exozodiacal dust and its connection with outer dust reservoirs remains unclear. Aims. We aim to explore the possible connection between hot ex…

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.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.SR2014★ 62 cited

Benchmark stars for Gaia: fundamental properties of the Population II star HD140283 from interferometric, spectroscopic and photometric data

O. Creevey, F. Thévenin, P. Berio +17

We determined the fundamental properties of HD 140283 by obtaining new interferometric and spectroscopic measurements and combining them with photometry from the literature. The in…

astro-ph.SR2014★ 37 cited

Improving the surface brightness-color relation for early-type stars using optical interferometry

M. Challouf, N. Nardetto, D. Mourard +18

The aim of this work is to improve the SBC relation for early-type stars in the color domain, using optical interferometry. Observations of eight B- and A-type…

astro-ph.SR2013★ 16 cited

The fundamental parameters of the roAp star 10 Aql

K. Perraut, S. Borgniet, M. Cunha +12

Due to the strong magnetic field and related abnormal surface layers existing in rapidly oscillating Ap stars, systematic errors are likely to be present when determining their eff…