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Autor Castro Rubio, Elisa de |
Documentos disponibles escritos por este autor (50)
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Gómez de Castro, Ana Inés ; López Santiago, Javier ; López Martínez, Fátima ; Sánchez, Néstor ; Castro Rubio, Elisa de ; Cornide, Manuel | Oxford Univ Press | 2015-06-01The Taurus-Auriga molecular complex (TMC) is the main laboratory for the study of low-mass star formation. The density and properties of interstellar dust are expected to vary across the TMC. These variations trace important processes such as du[...]![]()
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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 [...]![]()
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Caballero, J. A. ; López Santiago, Javier ; Castro Rubio, Elisa de ; Cornide Castro-Piñeiro, Manuel | IOP publishing ltd | 2009-01We used the Aladin Virtual Observatory tool and High Resolution Imager ROSAT archival data to search for X-ray variability in scale of days in 23 young stars in the ? Orionis cluster and a background galaxy. Five stars displayed unambiguous flar[...]![]()
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Caballero, J. A. ; López Santiago, J. ; Castro Rubio, Elisa de ; Cornide Castro-Piñeiro, Manuel | IOP publishing ltd | 2009-06We used the Aladin Virtual Observatory tool and High Resolution Imager ROSAT archival data to search for X-ray variability in scale of days in 23 young stars in the sigma Orionis cluster and a background galaxy. Five stars displayed unambiguous [...]![]()
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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[...]