Show simple item record

dc.contributor.authorLanza, A. F.en_GB
dc.contributor.authorAigrain, Suzanneen_GB
dc.contributor.authorMessina, S.en_GB
dc.contributor.authorLeto, G.en_GB
dc.contributor.authorPagano, I.en_GB
dc.contributor.authorAuvergne, M.en_GB
dc.contributor.authorBaglin, A.en_GB
dc.contributor.authorBarge, P.en_GB
dc.contributor.authorBonomo, A. S.en_GB
dc.contributor.authorCollier Cameron, A.en_GB
dc.contributor.authorCutispoto, G.en_GB
dc.contributor.authorDeleuil, M.en_GB
dc.contributor.authorDe Medeiros, J. R.en_GB
dc.contributor.authorFoing, B.en_GB
dc.contributor.authorMoutou, C.en_GB
dc.date.accessioned2009-12-03T15:33:08Zen_GB
dc.date.accessioned2011-01-25T11:54:10Zen_GB
dc.date.accessioned2013-03-20T13:15:38Z
dc.date.issued2009-03-05en_GB
dc.description.abstractAims. The space experiment CoRoT has recently detected a transiting hot Jupiter in orbit around a moderately active F-type mainsequence star (CoRoT-4a). This planetary system is of particular interest because it has an orbital period of 9.202 days, the second longest one among the transiting planets known to date. We study the surface rotation and the activity of the host star during an uninterrupted sequence of optical observations of 58 days. Methods. Our approach is based on a maximum entropy spot modelling technique extensively tested by modelling the variation in the total solar irradiance. It has been successfully applied to model the light curve of another active star with a transiting planet observed by CoRoT, i.e., CoRoT-2a. It assumes that stellar active regions consist of cool spots and bright faculae, analogous to sunspots and solar photospheric faculae, whose visibility is modulated by stellar rotation. Results. The modelling of the light curve of CoRoT-4a reveals three main active longitudes with lifetimes between ˜30 and ˜60 days that rotate quasi-synchronously with the orbital motion of the planet. The different rotation rates of the active longitudes are interpreted in terms of surface differential rotation, and a lower limit of 0.057 ± 0.015 is derived for its relative amplitude. The enhancement of activity observed close to the subplanetary longitude suggests a magnetic star-planet interaction, although the short duration of the time series prevents us from drawing definite conclusions. Conclusions. The present work confirms the quasi-synchronicity between stellar rotation and planetary orbital motion in the CoRoT-4 system and provides a lower limit for the surface differential rotation of the star. This information can be important in trying to understand the formation and evolution of this highly interesting planetary system. Moreover, there is an indication of a possible star-planet magnetic interaction that needs to be confirmed by future studies.en_GB
dc.identifier.citationVol. 506 (1), pp. 255-262en_GB
dc.identifier.doi10.1051/0004-6361/200811487en_GB
dc.identifier.urihttp://hdl.handle.net/10036/87333en_GB
dc.language.isoenen_GB
dc.publisherEDP Sciencesen_GB
dc.subjectstars: magnetic fieldsen_GB
dc.subjectstars: late-typeen_GB
dc.subjectstars: activityen_GB
dc.subjectstars: rotationen_GB
dc.subjectplanetary systemsen_GB
dc.titlePhotospheric activity and rotation of the planet-hosting star CoRoT-4aen_GB
dc.typeArticleen_GB
dc.date.available2009-12-03T15:33:08Zen_GB
dc.date.available2011-01-25T11:54:10Zen_GB
dc.date.available2013-03-20T13:15:38Z
dc.identifier.issn0004-6361en_GB
dc.identifier.issn1432-0746en_GB
pubs.declined2012-12-03T13:35:32.0+0000
dc.descriptionCopyright © The European Southern Observatory (ESO)en_GB
dc.identifier.journalAstronomy and Astrophysicsen_GB


Files in this item

This item appears in the following Collection(s)

Show simple item record