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Differential Rotation of CoRoT Stars and a Kepler Binary Star from Starspot Transit Mapping
DOI: 10.3847/1538-4357/ad66cb Bibcode: 2024ApJ...972...81V

Valio, Adriana; Araújo, Alexandre; Menezes, Fabian

While direct magnetic field measurements are rare for slowly rotating stars, spots observed during planetary transits provide a potential indicator of magnetic activity on stellar surfaces. Moreover, the rotation of the stellar surface can be probed by monitoring the spots' position with time in subsequent transits. This study investigates the dyn…

2024 The Astrophysical Journal
CoRoT 1
Exploring the Helium Core of the δ Scuti Star CoRoT 102749568 with Asteroseismology
DOI: 10.3847/1538-4357/834/2/146 Bibcode: 2017ApJ...834..146C

Li, Yan; Chen, Xinghao; Chen, Yanhui +2 more

Based on regularities in rotational splitting, we seek possible multiplets for the observed frequencies of CoRoT 102749568. There are 21 sets of multiplets identified, including four sets of multiplets with l = 1, nine sets of multiplets with l = 2, and eight sets of multiplets with l = 3. In particular, there are three complete triplets (f10…

2017 The Astrophysical Journal
CoRoT 10
The CoRoT Discovery of a Unique Triple-mode Cepheid in the Galaxy
DOI: 10.1088/2041-8205/795/2/L36 Bibcode: 2014ApJ...795L..36P

Poretti, E.; Baglin, A.; Weiss, W. W.

The exploitation of the CoRoT treasure of stars observed in the exoplanetary field allowed the detection of a unusual triple-mode Cepheid in the Milky Way, CoRoT 0223989566. The two modes with the largest amplitudes and a period ratio of 0.80 are identified with the first (P 1 = 1.29 days) and second (P 2 = 1.03 days) radial …

2014 The Astrophysical Journal
CoRoT 10
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
Evidence for Granulation in Early A-Type Stars
DOI: 10.1088/2041-8205/711/1/L35 Bibcode: 2010ApJ...711L..35K

Kallinger, Thomas; Matthews, Jaymie M.

Stars with spectral types earlier than about F0 on (or close) to the main sequence have long been believed to lack observable surface convection, although evolutionary models of A-type stars do predict very thin surface convective zones. We present evidence for granulation in two δ Scuti stars of spectral type A2: HD 174936 and HD 50844. Recent an…

2010 The Astrophysical Journal
CoRoT 68
Beaming Binaries: A New Observational Category of Photometric Binary Stars
DOI: 10.1086/521389 Bibcode: 2007ApJ...670.1326Z

Mazeh, Tsevi; Zucker, Shay; Alexander, Tal

The new photometric spaceborne survey missions COROT and Kepler will be able to detect minute flux variations in binary stars due to relativistic beaming caused by the line-of-sight motion of their components. In all but very short period binaries (P>10 days), these variations will dominate over the ellipsoidal and reflection periodic variabili…

2007 The Astrophysical Journal
CoRoT 144