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Variability in the CoRoT photometry of three hot O-type stars. HD 46223, HD 46150, and HD 46966
DOI: 10.1051/0004-6361/201116949 Bibcode: 2011A&A...533A...4B

Auvergne, M.; Gosset, E.; Baudin, F. +15 more

Context. The detection of pulsational frequencies in stellar photometry is required as input for asteroseismological modelling. The second short run (SRa02) of the CoRoT mission has provided photometric data of unprecedented quality and time-coverage for a number of O-type stars.
Aims: We analyse the CoRoT data corresponding to three hot O-ty…

2011 Astronomy and Astrophysics
CoRoT 102
Transiting exoplanets from the CoRoT space mission. XV. CoRoT-15b: a brown-dwarf transiting companion
DOI: 10.1051/0004-6361/201015276 Bibcode: 2011A&A...525A..68B

Mazeh, T.; Aigrain, S.; Alonso, R. +46 more

We report the discovery by the CoRoT space mission of a transiting brown dwarf orbiting a F7V star with an orbital period of 3.06 days. CoRoT-15b has a radius of 1.12+0.30-0.15 {R}_Jup and a mass of 63.3 ± 4.1 {M}_Jup, and is thus the second transiting companion lying in the theoretical mass domain of brown dwarfs. CoRoT-15b …

2011 Astronomy and Astrophysics
CoRoT 99
Accurate p-mode measurements of the G0V metal-rich CoRoT target HD 52265
DOI: 10.1051/0004-6361/201116547 Bibcode: 2011A&A...530A..97B

Auvergne, M.; Baudin, F.; García, R. A. +27 more

Context. The star HD 52265 is a G0V metal-rich exoplanet-host star observed in the seismology field of the CoRoT space telescope from November 2008 to March 2009. The satellite collected 117 days of high-precision photometric data on this star, showing that it presents solar-like oscillations. HD 52265 was also observed in spect…

2011 Astronomy and Astrophysics
CoRoT 96
An asteroseismic study of the O9V star HD 46202 from CoRoT space-based photometry
DOI: 10.1051/0004-6361/201015690 Bibcode: 2011A&A...527A.112B

Auvergne, M.; Baudin, F.; Michel, E. +13 more

The O9V star HD 46202, which is a member of the young open cluster NGC 2244, was observed by the CoRoT satellite in October/November 2008 during a short run of 34 days. From the very high-precision light curve, we clearly detect β Cep-like pulsation frequencies with amplitudes of ~0.1 mmag and below. A comparison with stellar models was performed …

2011 Astronomy and Astrophysics
CoRoT IUE 76
Amplitudes and lifetimes of solar-like oscillations observed by CoRoT. Red-giant versus main-sequence stars
DOI: 10.1051/0004-6361/201014037 Bibcode: 2011A&A...529A..84B

Goupil, M. -J.; Baudin, F.; Hatzes, A. P. +12 more

Context. The advent of space-borne missions such as CoRoT or Kepler providing photometric data has brought new possibilities for asteroseismology across the H-R diagram. Solar-like oscillations are now observed in many stars, including red giants and main-sequence stars.
Aims: Based on several hundred identified pulsating red giants, we aim t…

2011 Astronomy and Astrophysics
CoRoT 72
About the p-mode frequency shifts in HD 49933
DOI: 10.1051/0004-6361/201116633 Bibcode: 2011A&A...530A.127S

García, R. A.; Mathur, S.; Ballot, J. +2 more

We study the frequency dependence of the frequency shifts of the low-degree p modes measured in the F5V star HD 49933, by analyzing the second run of observations collected by the CoRoT satellite. The 137-day light curve is divided into two subseries corresponding to periods of low and high stellar activity. The activity-frequency relationship is …

2011 Astronomy and Astrophysics
CoRoT 48
Transiting exoplanets from the CoRoT space mission. XVIII. CoRoT-18b: a massive hot Jupiter on a prograde, nearly aligned orbit
DOI: 10.1051/0004-6361/201117192 Bibcode: 2011A&A...533A.130H

Mazeh, T.; Aigrain, S.; Alonso, R. +44 more

We report the detection of CoRoT-18b, a massive hot Jupiter transiting in front of its host star with a period of 1.9000693 ± 0.0000028 days. This planet was discovered thanks to photometric data secured with the CoRoT satellite combined with spectroscopic and photometric ground-based follow-up observations. The planet has a mass Mp = 3…

2011 Astronomy and Astrophysics
CoRoT 47
The CoRoT star 105288363: strong cycle-to-cycle changes of the Blazhko modulation
DOI: 10.1111/j.1365-2966.2011.18812.x Bibcode: 2011MNRAS.415.1577G

Poretti, E.; Szabó, R.; Kolenberg, K. +4 more

We present an analysis of the COnvection, ROtation and planetary Transits (CoRoT) star 105288363, a new Blazhko RR Lyrae star of type RRab (f0= 1.7623 d-1), observed with the CoRoT spacecraft during the second long run in the direction of the Galactic Centre (LRc02, time-base 145 d). The CoRoT data are characterized by an exc…

2011 Monthly Notices of the Royal Astronomical Society
CoRoT 44
Monitoring a high-amplitude δ Scuti star for 152 days: discovery of 12 additional modes and modulation effects in the light curve of CoRoT 101155310
DOI: 10.1051/0004-6361/201016045 Bibcode: 2011A&A...528A.147P

Auvergne, M.; Baudin, F.; Poretti, E. +12 more


Aims: The detection of small-amplitude nonradial modes in high-amplitude δ Sct (HADS) variables has been very elusive until at least five of them were detected in the light curve of V974 Oph obtained from ground-based observations. The combination of radial and nonradial modes has a high asteroseismic potential, thanks to the strong constrain…

2011 Astronomy and Astrophysics
CoRoT 43
Plaskett's star: analysis of the CoRoT photometric data
DOI: 10.1051/0004-6361/201014777 Bibcode: 2011A&A...525A.101M

Auvergne, M.; Gosset, E.; Baudin, F. +13 more

Context. The second short run (SRa02) of the CoRoT space mission for asteroseismology was partly devoted to stars belonging to the Mon OB2 association. An intense monitoring has been performed on Plaskett's star (HD 47129) and the unprecedented quality of the light curve allows us to shed new light on this very massive, non-eclipsing binary system…

2011 Astronomy and Astrophysics
CoRoT 38