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20072016
most citedFast core rotation in red-giant stars revealed by gravity-dominated mixed modes

511 citations · 3.7k across the 41 of their papers we have counts for

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10 papers · 1 filter

astro-ph2008★ 20 cited

MOST photometry of the enigmatic PMS pulsator HD 142666

K. Zwintz, T. Kallinger, D. B. Guenther +11

We present precise photometry of the pulsating Herbig Ae star HD 142666 obtained in two consecutive years with the MOST (Microvariability & Oscilations of STars) satellite. Previou…

astro-ph2008★ 34 cited

The nature of p-modes and granulation in HD 49933 observed by CoRoT

T. Kallinger, M. Gruberbauer, D. B. Guenther +2

Context: Recent observations of HD49933 by the space-photometric mission CoRoT provide photometric evidence of solar type oscillations in a star other than our Sun. The first publi…

astro-ph2008★ 4 cited

Oscillating red giants in the CoRoT exo-field: Asteroseismic mass and radius determination

T. Kallinger, W. W. Weiss, C. Barban +10

Context. Observations and analysis of solar-type oscillations in red-giant stars is an emerging aspect of asteroseismic analysis with a number of open questions yet to be explored.…

astro-ph2008★ 69 cited

On the detection of Lorentzian profiles in a power spectrum: A Bayesian approach using ignorance priors

M. Gruberbauer, T. Kallinger, W. W. Weiss +1

Aims. Deriving accurate frequencies, amplitudes, and mode lifetimes from stochastically driven pulsation is challenging, more so, if one demands that realistic error estimates be g…

astro-ph2008★ 24 cited

MOST photometry of the roAp star 10 Aql

D. Huber, H. Saio, M. Gruberbauer +12

Context: We present 31.2 days of nearly continuous MOST photometry of the roAp star 10Aql. Aims:The goal was to provide an unambiguous frequency identification for this little stud…

astro-ph2008★ 27 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-ph2007

Why are some A stars magnetic, while most are not?

G. A. Wade, J. Silvester, K. Bale +21

A small fraction of intermediate-mass main sequence (A and B type) stars have strong, organised magnetic fields. The large majority of such stars, however, show no evidence for mag…

astro-ph2007★ 296 cited

Weak magnetic fields in Ap/Bp stars: Evidence for a dipole field lower limit and a tentative interpretation of the magnetic dichotomy

M. Auriere, G. A. Wade, J. Silvester +22

We have investigated a sample of 28 well-known spectroscopically-identified magnetic Ap/Bp stars, with weak, poorly-determined or previously undetected magnetic fields, with the ai…

astro-ph2007

Cinderella - Comparison of INDEpendent RELative Least-squares Amplitudes

P. Reegen, M. Gruberbauer, L. Schneider +1

The identification of increasingly smaller signal from objects observed with a non-perfect instrument in a noisy environment poses a challenge for a statistically clean data analys…

astro-ph2007★ 68 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…