activity
20052020
most citedAsymptotic g modes: Evidence for a rapid rotation of the solar core

119 citations · 650 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.IM2020★ 1 cited

Dome C coherence time statistics from DIMM data

E. Aristidi, A. Agabi, L. Abe +3

We present a reanalysis of several years of DIMM data at the site of Dome C, Antarctica, to provide measurements of the coherence time . Statistics and seasonal behaviour of $…

astro-ph.IM2018★ 4 cited

Site testing study based on weather balloons measurements

E. Aristidi, A. Agabi, M. Azouit +8

We present wind and temperature profiles at Dome C measured by balloon born sonds during the polar summer. Data from 197 flights have been processed for 4 campaigns between 2000 an…

astro-ph.IM2018★ 24 cited

Monitoring the optical turbulence in the surface layer at Dome C, Antarctica, with sonic anemometers

Eric Aristidi, Jean Vernin, Eric Fossat +11

The optical turbulence above Dome C in winter is mainly concentrated in the first tens of meters above the ground. Properties of this so-called surface layer (SL) were investigated…

astro-ph.SR2017★ 119 cited

Asymptotic g modes: Evidence for a rapid rotation of the solar core

E. Fossat, P. Boumier, T. Corbard +11

We present the identification of very low frequency g modes in the asymptotic regime and two important parameters that have long been waited for: the core rotation rate, and the as…

astro-ph.SR2014★ 6 cited

Study of the sub-AU disk of the Herbig B[e] star HD 85567 with near-infrared interferometry

J. Vural, S. Kraus, A. Kreplin +5

Context: The structure of the inner disk of Herbig Be stars is not well understood. The continuum disks of several Herbig Be stars have inner radii that are smaller than predicted…

astro-ph.SR2013★ 78 cited

New insights into the dust formation of oxygen-rich AGB stars

I. Karovicova, M. Wittkowski, K. Ohnaka +3

We observed the AGB stars S Ori, GX Mon and R Cnc with the MIDI instrument at the VLTI. We compared the data to radiative transfer models of the dust shells, where the central stel…