{ "id": "1003.5802", "version": "v1", "published": "2010-03-30T12:25:28.000Z", "updated": "2010-03-30T12:25:28.000Z", "title": "Coronal properties of planet-bearing stars", "authors": [ "K. Poppenhaeger", "J. Robrade", "J. H. M. M. Schmitt" ], "comment": "accepted by A&A", "categories": [ "astro-ph.SR" ], "abstract": "Do extrasolar planets affect the activity of their host stars? Indications for chromospheric activity enhancement have been found for a handful of targets, but in the X-ray regime, conclusive observational evidence is still missing. We want to establish a sound observational basis to confirm or reject major effects of Star-Planet Interactions (SPI) in stellar X-ray emissions. We therefore conduct a statistical analysis of stellar X-ray activity of all known planet-bearing stars within 30pc distance for dependencies on planetary parameters such as mass and semimajor axis. We find that in our sample, there are no significant correlations of X-ray luminosity or the activity indicator L_X/L_bol with planetary parameters which cannot be explained by selection effects. Coronal SPI seems to be a phenomenon which might only manifest itself as a strong effect for a few individual targets, but not to have a major effect on planet-bearing stars in general.", "revisions": [ { "version": "v1", "updated": "2010-03-30T12:25:28.000Z" } ], "analyses": { "keywords": [ "planet-bearing stars", "coronal properties", "planetary parameters", "stellar x-ray emissions", "chromospheric activity enhancement" ], "tags": [ "journal article" ], "publication": { "doi": "10.1051/0004-6361/201014245", "journal": "Astronomy and Astrophysics", "year": 2010, "month": "Jun", "volume": 515 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 850652, "adsabs": "2010A&A...515A..98P" } } }