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Related papers: The CoRoT target HD175726: an active star with wea…

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HgMn Chemically Peculiar stars are among the quietest stars of the main-sequence. However, according to theoretical predictions, these stars could have pulsations related to the very strong overabundances of iron peak elements, which are…

Solar and Stellar Astrophysics · Physics 2015-05-13 G. Alecian , M. Gebran , M. Auvergne , O. Richard , R. Samadi , W. W. Weiss , A. Baglin

Solar-like oscillations are stochastically excited by turbulent convection at the surface layers of the stars. We study the role of the surface metal abundance on the efficiency of the stochastic driving in the case of the CoRoT target HD…

Solar and Stellar Astrophysics · Physics 2010-01-26 R. Samadi , H. -G. Ludwig , K. Belkacem , M. J. Goupil , M. -A. Dupret

The high performance photometric data obtained with space mission CoRoT offer the opportunity to efficiently constrain our models for the stellar interior of solar-like pulsating stars. On the occasion of the analysis of the oscillations of…

Solar and Stellar Astrophysics · Physics 2011-03-28 S. Deheuvels , E. Michel

Solar-like stars with an external convective envelope can develop magnetic activity cycles under the interaction of con- vection, rotation and magnetic fields. Even in the Sun, these dynamo effects are not yet well understood and it would…

Solar and Stellar Astrophysics · Physics 2015-03-17 R. A. Garcia , J. Ballot , S. Mathur , D. Salabert , C. Regulo

Context. The CoRoT mission, a pioneer in exoplanet searches from space, has completed its first 150 days of continuous observations of ~12000 stars in the galactic plane. An analysis of the raw data identifies the most promising candidates…

About 30.5 days of nearly uninterrupted broadband photometry of the solar-type star Kappa1 Ceti, obtained with the MOST (Microvariability & Oscillations of STars) satellite, shows evidence for two large starspots with different rotation…

We present the discovery of a candidate multiply-transiting system, the first one found in the CoRoT mission. Two transit-like features with periods of 5.11 and 11.76d are detected in the CoRoT light curve, around a main sequence K1V star…

We present the CoRoT light curve of the bright B2.5V star HD 48977 observed during a short run of the mission in 2008, as well as a high-resolution spectrum gathered with the HERMES spectrograph at the Mercator telescope. We use several…

We present the analysis of the time series observations of CoRoT\,102699796 obtained by the CoRoT satellite that show the presence of five independent oscillation frequencies in the range 3.6-5 c/d. Using spectra acquired with FLAMES@VLT,…

Solar and Stellar Astrophysics · Physics 2015-05-28 V. Ripepi , F. Cusano , M. Di Criscienzo , G. Catanzaro , F. Palla , M. Marconi , P. Ventura , C. Neiner , C. Catala , S. Bernabei

Low amplitude is the defining characteristic of solar-like oscillations. The space projects $Kepler$ and $CoRoT$ give us a great opportunity to successfully detect such oscillations in numerous targets. Achievements of asteroseismology…

Solar and Stellar Astrophysics · Physics 2015-06-19 M. Yıldız , Z. Çelik Orhan , Ç. Aksoy , S. Ok

The CoRoT satellite is collecting precise time-resolved photometry for tens of asteroseismology targets. To ensure a correct interpretation of the CoRoT data, the atmospheric parameters, chemical compositions, and rotational velocities of…

Solar and Stellar Astrophysics · Physics 2015-05-13 E. Niemczura , T. Morel , C. Aerts

Context. The PLAnetary Transits and Oscillations of stars (PLATO) mission will observe the same area of the sky continuously for at least two years in an effort to detect transit signals of an Earth-like planet orbiting a solar-like star.…

Earth and Planetary Astrophysics · Physics 2024-10-29 A. F. Krenn , M. Lendl , S. Sulis , M. Deleuil , S. J. Hofmeister , N. Jannsen , L. Fossati , J. De Ridder , D. Seynaeve , R. Jarolim , A. M. Veronig

Context: We present the results of an extensive ground-based photometric and spectroscopic campaign on the gamma Dor CoRoT target HD49434. This campaign was preparatory to the CoRoT satellite observations, which took place from October 2007…

Six O-type stars were observed continuously by the CoRoT satellite during a 34.3-day run. The unprecedented quality of the data allows us to detect even low-amplitude stellar pulsations in some of these stars (HD 46202 and the binaries HD…

Classical Be stars are rapid rotators of spectral type late O to early A and luminosity class V-III, wich exhibit Balmer emission lines and often a near infrared excess originating in an equatorially concentrated circumstellar envelope,…

Stellar activity cycles are the manifestation of dynamo process running in the stellar interiors. They have been observed during years to decades thanks to the measurement of stellar magnetic proxies at the surface of the stars such as the…

Solar and Stellar Astrophysics · Physics 2015-06-12 S. Mathur , R. A. Garcia , A. Morgenthaler , D. Salabert , P. Petit , J. Ballot , C. Regulo , C. Catala

The Be star 102719279 is an interesting target observed with CoRoT during two runs, giving us the possibility to study the stability of the detected frequencies and to search for any correlation with outburts, as it was recently found in…

Solar and Stellar Astrophysics · Physics 2010-10-12 J. Gutiérrez-Soto , T. Semaan , R. Garrido , F. Baudin , A. -M. Hubert , C. Neiner

Oscillations of the Sun have been used to understand its interior structure. The extension of similar studies to more distant stars has raised many difficulties despite the strong efforts of the international community over the past…

Astrophysics · Physics 2010-11-11 E. Michel , A. Baglin , M. Auvergne , C. Catala , R. Samadi

The space experiment CoRoT has recently detected a transiting hot Jupiter in orbit around a moderately active F-type main-sequence star (CoRoT-Exo-4a). This planetary system is of particular interest because it has an orbital period of…

Long timeseries of data increase the frequency resolution in the power spectrum. This allows for resolving stochastically excited modes with long mode lifetimes, as well as features that are close together in frequency. The CoRoT fields…

Solar and Stellar Astrophysics · Physics 2015-05-19 S. Hekker , C. Barban , F. Baudin , J. De Ridder , T. Kallinger , T. Morel , W. J. Chaplin , Y. Elsworth
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