activity
20062008
most citedMOST photometry of the RRd Lyrae variable AQ Leo: Two radial modes, 32 combination frequencies, and beyond

68 citations · 159 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph20083 cited

The seismology programme of CoRoT

E. Michel, A. Baglin, M. Auvergne +1

We introduce the main lines and specificities of the CoRoT Seismology Core Programme. The development and consolidation of this programme has been made in the framework of the CoRo…

astro-ph2008

Solar-like oscillations in red giants in the CoRoT exo-field

S. Hekker, C. Barban, T. Kallinger +4

Asteroseismic observations from space can provide us with long time series of uninterrupted high quality data for many stars at the same time. The CoRoT satellite (Convection Rotat…

astro-ph200827 cited

MOST photometry and modeling of the rapidly oscillating (roAp) star gamma Equ

M. Gruberbauer, H. Saio, D. Huber +9

Aims. Despite photometry and spectroscopy of its oscillations obtained over the past 25 years, the pulsation frequency spectrum of the rapidly oscillating Ap (roAp) star gamma Equ…

astro-ph200731 cited

MOST photometry and DDO spectroscopy of the eclipsing (white dwarf + red dwarf) binary V471 Tau

Krzysztof Z. Kaminski, Slavek M. Rucinski, Jaymie M. Matthews +7

The Hyades K2V+WD system 471 Tau is a prototype post-common envelope system and a likely cataclysmic binary progenitor. We present 10 days of nearly continuous optical photometry b…

astro-ph200768 cited

MOST photometry of the RRd Lyrae variable AQ Leo: Two radial modes, 32 combination frequencies, and beyond

Michael Gruberbauer, Katrien Kohlenberg, Jason F. Rowe +12

Highly precise and nearly uninterrupted optical photometry of the RR Lyrae star AQ Leo was obtained with the MOST (Microvariability & Oscillations of STars) satellite over 34.4 day…

astro-ph200630 cited

Line profile variations in rapidly oscillating Ap stars: resolution of the enigma

O. Kochukhov, T. Ryabchikova, W. W. Weiss +2

We have carried out the first survey of the pulsational line profile variability in rapidly oscillating Ap (roAp) stars. We analysed high signal-to-noise time-series observations o…