{ "id": "1009.1173", "version": "v1", "published": "2010-09-06T22:51:57.000Z", "updated": "2010-09-06T22:51:57.000Z", "title": "Analysis of variability of TW Hya as observed by MOST and ASAS in 2009", "authors": [ "Michal Siwak", "Slavek M. Rucinski", "Jaymie M. Matthews", "Grzegorz Pojmanski", "Rainer Kuschnig", "David B. Guenther", "Anthony F. J. Moffat", "Dimitar Sasselov", "Werner W. Weiss" ], "comment": "Accepted to MNRAS", "categories": [ "astro-ph.SR" ], "abstract": "As a continuation of our previous studies in 2007 and 2008, new photometric observations of the T Tauri star TW Hya obtained by the MOST satellite and the ASAS project over 40 days in 2009 with temporal resolution of 0.2 days are presented. A wavelet analysis of the combined MOST-ASAS data provides a rich picture of coherent, intermittent, variable-period oscillations, similarly as discovered in the 2008 data. The periods (1.3 - 10 days) and systematic period shortening on time scales of weeks can be interpreted within the model of magneto-rotationally controlled accretion processes in the inner accretion disk around the star. Within this model and depending on the assumed visibility of plasma parcels causing the oscillations, the observed shortest-period oscillation period may indicate the stellar rotation period of 1.3 or 2.6 d, synchronized with the disk at 4.5 or 7.1 solar radii, respectively.", "revisions": [ { "version": "v1", "updated": "2010-09-06T22:51:57.000Z" } ], "analyses": { "keywords": [ "variability", "tauri star tw hya", "shortest-period oscillation period", "inner accretion disk", "stellar rotation period" ], "tags": [ "journal article" ], "publication": { "doi": "10.1111/j.1365-2966.2010.17649.x", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2011, "month": "Feb", "volume": 410, "number": 4, "pages": 2725 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 868164, "adsabs": "2011MNRAS.410.2725S" } } }