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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
An analysis of CoRoT multicolour photometry of exoplanets
DOI: 10.1093/mnras/sts087 Bibcode: 2013MNRAS.428..891B

Poretti, E.; Borsa, F.

We analysed the chromatic data of the planetary transits observed with CoRoT to supply homogeneous time series in each of the CoRoT colours. In a first step, we cleaned the chromatic light curves from the contamination of nearby stars and removed outliers and trends caused by anything different from the planetary transits. Then, we simultaneously …

2013 Monthly Notices of the Royal Astronomical Society
CoRoT 8
Attempt to detect the granulation signature in the HgMn star HD 175640 from CoRoT light curves
DOI: 10.1093/mnras/stt1339 Bibcode: 2013MNRAS.435.1852G

Alecian, G.; Ghazaryan, S.; Harutyunian, H.

HgMn stars are affected by atomic diffusion processes. Because theoretical models based on atomic diffusion require that the atmospheres of ApBp stars have to be much more stable than those of normal stars, the detection or the absence of detection of granulation in them should be an interesting information for the modelling. We would like to addr…

2013 Monthly Notices of the Royal Astronomical Society
CoRoT 5