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[PDF] Top 20 Rotation period distribution of CoRoT and Kepler Sun-like stars

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Rotation period distribution of CoRoT and Kepler Sun-like stars

Rotation period distribution of CoRoT and Kepler Sun-like stars

... occurrence of young stars, cor- responding to group I, compared to group ...fewer stars are observed with an increasing period is explained by a detectability ...its period increases. ... See full document

13

The variability behaviour of CoRoT M-giant stars

The variability behaviour of CoRoT M-giant stars

... amplitude of stochastically excited solar-type oscillations, which is typical of the GK-type giants, progress to a mixture of Mira-like and solar-like vari- ability, as found in ... See full document

11

The variability behaviour of CoRoT M-giant stars

The variability behaviour of CoRoT M-giant stars

... amplitude of stochastically excited solar-type oscillations, which is typical of the GK-type giants, progress to a mixture of Mira-like and solar-like vari- ability, as found in ... See full document

11

Photospheric activity and rotation of the planet-hosting star CoRoT-4a

Photospheric activity and rotation of the planet-hosting star CoRoT-4a

... differential rotation found through our spot mod- elling is not remarkably dependent on the adopted value of the facular-to-spotted area ratio Q and is at least 6 −7 times that de- rived for ... See full document

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Magnetic activity in the photosphere of CoRoT-Exo-2a: Active longitudes and short-term spot cycle in a young Sun-like star

Magnetic activity in the photosphere of CoRoT-Exo-2a: Active longitudes and short-term spot cycle in a young Sun-like star

... variation of the spotted area does not depend on the inclusion of the faculae in the model and its period can be considered as a robust ...amplitude of the light curve modulation in ... See full document

8

Stellar cycles from photometric data: CoRoT stars

Stellar cycles from photometric data: CoRoT stars

... yr and 2.4 yr computed here are compati- ble with the typical time scales of 1 ...yr and 2.8 yr, respectively, of the so-called Gnevyshev gaps ( Gnevyshev 1963 , 1967 , 1977 ...phase of ... See full document

7

Debris disks among Kepler solar rotational analog stars

Debris disks among Kepler solar rotational analog stars

... Observations of circumstellar disks provide a powerful tool for our understanding of planetary system ...collision of the remaining solid material of the planet formation ...presence of ... See full document

9

New suns in the cosmos. IV. The multifractal nature of stellar magnetic activity in kepler cool stars

New suns in the cosmos. IV. The multifractal nature of stellar magnetic activity in kepler cool stars

... deviation of the subseries de fined by k- rotation periods (hereafter S á ph, k ñ), where k=5 is ...values of S á ph, k ñ extracted from Mathur et ...scales of order or higher than the ... See full document

13

Fundamental parameters of Be stars located in the seismology fields of COROT

Fundamental parameters of Be stars located in the seismology fields of COROT

... fast and solid-body-type rotation flattens the star, causing a gravitational darkening of the stel- lar surface due to the variation of the temperature and den- sity distribution ... See full document

25

Interplay of tidal evolution and stellar wind braking in the rotation of stars hosting massive close-in planets

Interplay of tidal evolution and stellar wind braking in the rotation of stars hosting massive close-in planets

... application of the creep tide theory (Ferraz-Mello) to the study of the rotation of stars hosting massive close-in ...The stars have nearly the same tidal relaxation factors as ... See full document

12

Kepler rapidly rotating giant stars

Kepler rapidly rotating giant stars

... giant stars are relatively rare and may represent important stages of stellar evolution, resulting from stellar coalescence of close binary systems or accretion of substellar companions ... See full document

6

Rotação e atividade de estrelas F, G e K observadas pelos satélites CoRoT e Kepler

Rotação e atividade de estrelas F, G e K observadas pelos satélites CoRoT e Kepler

... question of how singular the Sun appears to be when compared to a class of solar-like stars in terms of their activity and rotation has been the subject of ... See full document

111

Testing the recovery of stellar rotation signals from Kepler light curves using a blind hare-and-hounds exercise

Testing the recovery of stellar rotation signals from Kepler light curves using a blind hare-and-hounds exercise

... deviation of the periods mea- sured from each quarter was then ...only stars with long lived variability are accepted, thus increas- ing the likelihood that the reported periods are ...remaining ... See full document

16

Rotation periods and ages of solar analogs and solar twins revealed by the kepler mission

Rotation periods and ages of solar analogs and solar twins revealed by the kepler mission

... SURFACE ROTATION RATES The average surface P rot is obtained from light curve modula- tion ...PDC-MAP and sim- ple aperture photometry light curves (Christiansen et ...drifts, and discontinuities ... See full document

5

Lithium abundance and rotation of seismic solar analogues: solar and stellar connection from Kepler and Hermes observations

Lithium abundance and rotation of seismic solar analogues: solar and stellar connection from Kepler and Hermes observations

... , and references ...a rotation-lithium relation exists even at an age of 5 Myr and also exhibits a significant ...depletion and the rotational history of exoplanet-host ... See full document

11

The rotational behavior of kepler stars with planets

The rotational behavior of kepler stars with planets

... missions CoRoT (Baglin et al. 2007 ) and Kepler (Koch et ...study of the behavior of stellar rotation, including the rotation of stars with planets, by ... See full document

11

Wavelets: a powerful tool for studying rotation, activity, and pulsation in Kepler and CoRoT stellar light curves

Wavelets: a powerful tool for studying rotation, activity, and pulsation in Kepler and CoRoT stellar light curves

... modulation of the star was related to two active longi- tudes initially on opposite hemispheres, ...a rotation period of 4 .522±0.0024 days, and the other slowly migrates (retrograde ... See full document

10

Rotation and magnetism of Kepler pulsating solar-like stars: towards asteroseismically calibrated age-rotation relations

Rotation and magnetism of Kepler pulsating solar-like stars: towards asteroseismically calibrated age-rotation relations

... developed and refined by works such as Pace & Pasquini ( 2004 ), Barnes ( 2007 ), Cardini & Cassatella ( 2007 ), Mamajek & Hillenbrand ( 2008 ), Meibom et ...), and Chanamé & Ramírez ( 2012 ... See full document

15

Activity and rotation of Kepler-17

Activity and rotation of Kepler-17

... the Sun, spots can be seen throughout the disk, at different longitudes and latitudes that change over the course of the magnetic ...late-type stars and is believed to be generated by ... See full document

6

New Suns in the Cosmos II: differential rotation in Kepler Sun-like stars

New Suns in the Cosmos II: differential rotation in Kepler Sun-like stars

... coherence of a photometric signal can be estimated by the relative height of successive peaks in the ACF (Lanza et ...17 stars presenting unambiguous stable photometric signals, indicating rotational ... See full document

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