Multi-wavelength observing of a forming solar-like star

S. G. Gregory, E. Flaccomio, C. Argiroffi, J. Bouvier, J. -F. Donati, E. D. Feigelson, K. V. Getman, G. A. J. Hussain, M. Jardine, F. M. Walter

Research output: Chapter in Book/Report/Conference proceedingConference contribution


V2129 Oph is a 1.35 solar mass classical T Tauri star, known to possess a strong and complex magnetic field. By extrapolating from an observationally derived magnetic surface map, obtained through Zeeman-Doppler imaging, models of V2129 Oph's corona have been constructed, and used to make predictions regarding the global X-ray emission measure, the amount of modulation of X-ray emission, and the density of accretion shocks. In late June 2009 we will under take an ambitious multi-wavelength, multi-observing site, and near contemporaneous campaign, combining spectroscopic optical, nIR, UV, X-ray, spectropolarimetric and photometric monitoring. This will allow the validity of the 3D field topologies derived via field extrapolation to be determined.
Original languageUndefined/Unknown
Title of host publicationMulti-wavelength observing of a forming solar-like star
Publication statusPublished - 26 Jun 2009

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