S. Sciortino, G. Rauw, M. Audard, C. Argiroffi, Y. -H. Chu, M. De Becker, J. Drake, E. Feigelson, E. Gosset, N. Grosso, M. Güdel, M. Guerrero, A. Hervé, J. Kastner, R. Montez, Y. Nazé, L. Oskinova, B. Stelzer, A. ud-Doula
Stars over a wide range of masses and evolutionary stages are nowadays known to emit X-rays. This X-ray emission is a unique probe of the most energetic phenomena occurring in the circumstellar environment of these stars, and provides precious insight on magnetic phenomena or hydrodynamic shocks. Owing to its large collecting area, Athena+ will open up an entirely new window on these phenomena. Indeed, Athena+ will not only allow us to study many more objects with an unprecedented spectral resolution, but will also pioneer the study of the dynamics of these objects via time-resolved high-resolution spectroscopy. In this way, Athena+ will be a unique tool to study accretion processes in TTauri stars, flaring activity in young stars, dynamos in ultra-cool dwarfs, small and large-scale structures in the winds of single massive stars, wind interactions in massive binary systems, hot bubbles in planetary nebula... All these studies will lead to a deeper understanding of yet poorly understood processes which have profound impact in star and planetary system formation as well as in feedback processes on Galactic scale.
View original:
http://arxiv.org/abs/1306.2333
No comments:
Post a Comment