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Montes Gutiérrez, David ; Castro Rubio, Elisa de ; Gómez de Castro, Ana Inés ; Canet Varea, Ada ; Beitia Antero, Leire ; Gómez Marfil, Emilio | 2021-01-18El objetivo principal del proyecto de innovación docente es reforzar las habilidades técnicas (soft skills) de los alumnos de astrofísica del Grado en Física y Matemáticas y del Máster en Astrofísica de la Facultad. De cara a los Trabajos Fin de[...]texto impreso
This contribution gathers the contents of the white paper submitted by the UV community to the Call issued by the European Space Agency in March 2013, for the definition of the L2 and L3 missions in the ESA science program. We outlined the key s[...]texto impreso
The atmospheric structure of T Tauri stars (TTSs) and its connection with the large-scale outflow is poorly known. Neither the effect of the magnetically mediated interaction between the star and the disc is well understood. The Mg II multiplet [...]texto impreso
Barderas, Gonzalo ; Romero Pérez, Mª Pilar ; Goicoechea, S. | Universidad Complutense de Madrid | 2016La Misión ExoMars16 es la primera misión del programa ExoMars de la ESA, cuyo lanzamiento se realizó el día 14 de marzo de 2016 estando prevista su llegada a Marte en octubre de 2016. Esta misión consta del módulo orbital Gas Tracer Orbiter y de[...]texto impreso
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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
Gómez de Castro, Ana Inés ; López Santiago, Javier ; López Martínez, Fátima ; Sánchez, Néstor ; Sestito, Paola ; Castro Rubio, Elisa de ; Cornide, Manuel ; Yáñez, Javier | IOP Publishing | 2015-02In this work, we identify 63 bona fide new candidates to T Tauri stars (TTSs) in the Taurus-Auriga region using as baseline its ultraviolet excess. The initial data set has been defined from the GALEX all sky survey (AIS). The GALEX satellite ob[...]texto impreso
Magdaleno, S. ; Cueto, M. ; Herraiz, M. ; Rodríguez Caderot, Gracia ; Sardon, E. ; Rodríguez, I. | Elsevier | 2013-04Plasma depletions (or bubbles) are strong reductions in the ionospheric F-region plasma density due to the appearance of a Rayleigh-Taylor instability in the post-sunset, producing severe radio signal disruptions when crossing them. Most of the [...]texto impreso
Gómez de Castro, Ana Inés ; Sánchez, Néstor ; Sestito, Paola ; Rodríguez, Pablo ; Teresa Gómez, Maite ; Seijas, Juan ; López-Martinez, Fátima ; Quintana, Jose ; Ubierna, Marcos ; Muñoz, Jacinto | Society of Photo-Optical Instrumentation Engineers (SPIE) | 2012-09ISSIS is the Imaging and Slitless Spectroscopy Instrument for the World Space Observatory - Ultraviolet (WSO-UV), a 170 cm space telescope to be launched in late 2015. ISSIS is a multipurpose instrument designed to carry out high resolution and [...]texto impreso
Armengot, Marcelo ; Sánchez, N. ; López Santiago, Javier ; Gómez de Castro, Ana Inés | Springer | 2014-11Large sky surveys are providing a huge amount of information for studies of the interstellar medium, the galactic structure or the cosmic web. Setting into a common frame information coming from different wavelengths, over large fields of view, [...]texto impreso
Sánchez Cano, B. ; Radicella, S. M. ; Herraiz, M. ; Witasse, O. ; Rodríguez Caderot, Gracia | Elsevier Science B.V., Amsterdam | 2013Several models of the martian ionosphere have been developed in the last years. In this paper, a new empirical model for the dayside electron density of the martian ionosphere (primary and secondary layer), called NeMars, is described. The model[...]texto impreso
Barderas, Gonzalo ; Romero Pérez, Mª Pilar ; Vázquez Martínez, Luis ; Vázquez Poletti, José Luis ; Llorente, I. M. | Wiley | 2012-11We have generated predictions for observing Phobos transits during the period 2012–2014 using the Mars Science Laboratory. We describe how the detections of Phobos eclipses can be used as an alternative procedure to determine the coordinates of [...]texto impreso
Astronomical surveys provide an amazing amount of information for the understanding of specific astrophysical problems, from the large scale structure of galaxy clusters, to the formation of stars. Large scale surveys are often complemented with[...]