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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
Combi, J. A. ; Albacete Colombo, J. F. ; López Santiago, J. ; Romero, G. E. ; Sánchez Ayaso, E. ; Marti, J. ; Luque Escamilla, P. L. ; Pérez González, Pablo Guillermo ; Muñoz Arjonilla,, A. J. ; Sánchez Sutil, J. R. | EDP Sciencies | 2010-11Aims. We report results of an X-ray study of the supernova remnant (SNR) G344.7-0.1 and the point-like X-ray source located at the geometrical center of the SNR radio structure. Methods. The morphology and spectral properties of the remnant and [...]texto impreso
López García, M. A. ; López Santiago, J. ; Albacete Colombo, J. F. ; Pérez González, Pablo Guillermo ; Castro Rubio, Elisa de | Wiley | 2013-02Nearby star-forming regions are ideal laboratories to study high-energy emission of different stellar populations, from very massive stars to brown dwarfs. NGC 2023 is a reflection nebula situated to the south of the Flame Nebula (NGC 2024) and [...]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, 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 [...]texto impreso
Sánchez Ayaso, E. ; Combi, J. A. ; Bocchino, F. ; Albacete Colombo, J. F. ; López Santiago, J. ; Marti, J. ; Castro Rubio, Elisa de | EDP Sciencies | 2013-04Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray emitting plasma of the supernova remnant G272.2-3.2 in order to obtain important constraints on its ionization stage, the progenitor supernova ex[...]
