Search Publications

Rotation in NGC 2264: a study based on CoRoT photometric observations
DOI: 10.1093/mnras/stt003 Bibcode: 2013MNRAS.430.1433A

Bouvier, J.; Micela, G.; Favata, F. +2 more

Rotation is one of the key stellar parameters which undergo substantial evolution during the stellar lifetime, in particular during the early stages. Stellar rotational periods can be determined on the basis of the periodic modulation of starlight produced by non-uniformities on the surface of the stars, due to manifestation of stellar activity. W…

2013 Monthly Notices of the Royal Astronomical Society
CoRoT 67
CoRoT: Harvest of the exoplanet program
DOI: 10.1016/j.icarus.2013.03.022 Bibcode: 2013Icar..226.1625M

Guillot, Tristan; Cabrera, Juan; Deeg, Hans J. +6 more

One of the objectives of the CoRoT mission is the search for transiting extrasolar planets using high-precision photometry, and the accurate characterization of their fundamental parameters. The CoRoT satellite consecutively observes crowded stellar fields since February 2007, in high-cadence precise photometry; periodic eclipses are detected and …

2013 Icarus
CoRoT 58
An in-depth study of HD 174966 with CoRoT photometry and HARPS spectroscopy. Large separation as a new observable for δ Scuti stars
DOI: 10.1051/0004-6361/201220256 Bibcode: 2013A&A...559A..63G

Auvergne, M.; Amado, P. J.; Baudin, F. +18 more


Aims: The aim of this work was to use a multi-approach technique to derive the most accurate values possible of the physical parameters of the δ Sct star HD 174966, which was observed with the CoRoT satellite. In addition, we searched for a periodic pattern in the frequency spectra with the goal of using it to determine the mean density of th…

2013 Astronomy and Astrophysics
CoRoT 56
CoRoT 102918586: a γ Doradus pulsator in a short-period eccentric eclipsing binary
DOI: 10.1051/0004-6361/201220755 Bibcode: 2013A&A...552A..60M

Gandolfi, D.; Rainer, M.; Montalbán, J. +2 more

Pulsating stars in eclipsing binary systems are powerful tools to test stellar models. Binarity enables us to constrain the pulsating component's physical parameters and this knowledge drastically improves the input physics for asteroseismic studies. The study of stellar oscillations then allows us to improve our understanding of stellar interiors…

2013 Astronomy and Astrophysics
CoRoT 42
Overview of semi-sinusoidal stellar variability with the CoRoT satellite
DOI: 10.1051/0004-6361/201219415 Bibcode: 2013A&A...555A..63D

Baglin, A.; Catelan, M.; Janot-Pacheco, E. +13 more

Context. To date, the CoRoT space mission has produced more than 124 471 light curves. Classifying these curves in terms of unambiguous variability behavior is mandatory for obtaining an unbiased statistical view on their controlling root-causes.
Aims: The present study provides an overview of semi-sinusoidal light curves observed by the CoRo…

2013 Astronomy and Astrophysics
CoRoT 37
γ Doradus pulsation in two pre-main sequence stars discovered by CoRoT
DOI: 10.1051/0004-6361/201220127 Bibcode: 2013A&A...550A.121Z

Chaintreuil, S.; Ryabchikova, T.; Fossati, L. +5 more

Context. Pulsations in pre-main sequence stars have been discovered several times within the last years. But nearly all of these pulsators are of δ Scuti-type. γ Doradus-type pulsation in young stars has been predicted by theory, but lack observational evidence.
Aims: We present the investigation of variability caused by rotation and (γ Dorad…

2013 Astronomy and Astrophysics
CoRoT 32
CoRoT 101186644: A transiting low-mass dense M-dwarf on an eccentric 20.7-day period orbit around a late F-star. Discovered in the CoRoT lightcurves
DOI: 10.1051/0004-6361/201220862 Bibcode: 2013A&A...553A..30T

Mazeh, T.; Alonso, R.; Bouchy, F. +10 more

We present the study of the CoRoT transiting planet candidate 101186644, also named LRc01_E1_4780. Analysis of the CoRoT lightcurve and the HARPS spectroscopic follow-up observations of this faint (mV = 16) candidate revealed an eclipsing binary composed of a late F-type primary (Teff = 6090 ± 200 K) and a low-mass, dense lat…

2013 Astronomy and Astrophysics
CoRoT 27
Secondary eclipses in the CoRoT light curves. A homogeneous search based on Bayesian model selection
DOI: 10.1051/0004-6361/201220081 Bibcode: 2013A&A...550A..67P

Deeg, H. J.; Parviainen, H.; Belmonte, J. A.


Aims: We aim to identify and characterize secondary eclipses in the original light curves of all published CoRoT planets using uniform detection and evaluation critetia.
Methods: Our analysis is based on a Bayesian model selection between two competing models: one with and one without an eclipse signal. The search is carried out by mappi…

2013 Astronomy and Astrophysics
CoRoT 25
The Future of the Sun: An Evolved Solar Twin Revealed by CoRoT
DOI: 10.1088/2041-8205/771/2/L31 Bibcode: 2013ApJ...771L..31D

Porto de Mello, G. F.; Castro, M.; da Costa, J. S. +3 more

The question of whether the Sun is peculiar within the class of solar-type stars has been the subject of active investigation over the past three decades. Although several solar twins have been found with stellar parameters similar to those of the Sun (albeit in a range of Li abundances and with somewhat different compositions), their rotation per…

2013 The Astrophysical Journal
CoRoT 22
New Suns in the Cosmos?
DOI: 10.1088/2041-8205/773/2/L18 Bibcode: 2013ApJ...773L..18D

Catelan, M.; Ferreira Lopes, C. E.; De Medeiros, J. R. +5 more

The present work reports on the discovery of three stars that we have identified to be rotating Sun-like stars, based on rotational modulation signatures inferred from light curves from the CoRoT mission's Public Archives. In our analysis, we performed an initial selection based on the rotation period and position in the period-T eff di…

2013 The Astrophysical Journal
CoRoT 20