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López Santiago, Javier ; Miceli, M. ; Valle, M. V. del ; Romero, G. E. ; Bonito, R. ; Albacete Colombo, J. F. ; Pereira, V. ; Castro Rubio, Elisa de ; Damiani, F. | IOP Publishing | 2012-09-20Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow shocks have been detected in the mid-infrared for several high-mass runaway stars and in radio waves for one star. Theoretical models predict the[...]texto impreso
López Santiago, Javier ; Peri, C. S. ; Bonito, R. ; Miceli, M. ; Albacete Colombo, J. F. ; Benaglia, P. ; Castro Rubio, Elisa de | IOP Publishing | 2013-10-20Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km s^-1, creating strong shocks when interacting with the interstellar medium. Several cases of jets h[...]texto impreso
López-Santiago, Javier ; Peri, C.S. ; Bonito, R. ; Miceli, M. ; Albacete Colombo, J.F. ; Benaglia, P. ; De Castro, E. | IOP Publishing | 2013-10Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km/s, creating strong shocks when interacting with interstellar medium. Several cases of jets have bee[...]texto impreso
Ustamujic, S. ; Orlando, S. ; Bonito, R. ; Miceli, M. ; Gómez de Castro, Ana Inés ; López Santiago, J. | EDP Sciences | 2016Context. X-ray observations of protostellar jets show evidence of strong shocks heating the plasma up to temperatures of a few million degrees. In some cases, the shocked features appear to be stationary. They are interpreted as shock diamonds. [...]texto impreso
Pereira Blanco, Víctor ; López Santiago, J. ; Miceli, M. ; Bonito, R. ; Castro Rubio, Elisa de | EDP Sciencies | 2016-04Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serve as particle acceleration sites. Previous theoretical mode[...]texto impreso
Pereira, V. ; López Santiago, J. ; Miceli, M. ; Bonito, R. ; Castro Rubio, Elisa de | EDP Sciencies | 2016-04Context. Runaway O- and early B-type stars passing through the interstellar medium at supersonic velocities and characterized by strong stellar winds may produce bow shocks that can serve as particle acceleration sites. Previous theoretical mode[...]texto impreso
Miceli, M. ; Orlando, S. ; Pereira Blanco, Víctor ; Acero, F. ; Katsuda, S. ; Decourchelle, A. ; Winkler, F.P. ; Bonito, R. ; Reale, F. ; Pérès, G. ; Li, J. ; Dubner, G. | EDP Sciencies | 2016-09Context. The supernova remnant SN 1006 is a source of high-energy particles and its southwestern limb is interacting with a dense ambient cloud, thus being a promising region for ??ray hadronic emission. Aims. We aim at describing the physics an[...]texto impreso
López Santiago, J. ; Bonito, R. ; Orellana, M. ; Miceli, M. ; Orlando, S. ; Ustamujic, S. ; Albacete Colombo, J. F. ; Castro Rubio, Elisa de ; Gómez de Castro, Ana Inés | American Astronomical Society | 2015-06-10We investigate the plausibility of detecting X-ray emission from a stellar jet that impacts a dense molecular cloud, a scenario that may be typical for classical T Tauri stars with jets in dense star-forming complexes. We first model the impact [...]
