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Autor López Martínez, Fátima |
Documentos disponibles escritos por este autor (9)
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The C ii] feature at similar to 2325 angstrom is very prominent in the spectra of T Tauri stars (TTSs). This feature is a quintuplet of semiforbidden transitions excited at electron temperatures around 10 000 K that, together with the nearby Si [...]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
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
Gómez de Castro, Ana I. ; López Santiago, Javier ; López Martínez, Fátima ; Sánchez, Néstor ; Sestito, Paola ; Castro Rubio, Elisa de ; Cornide Castro-Piñeiro, Manuel ; Yáñez Gestoso, Javier | University Chicago Press | 2015-02In this work, we identify 63 bona fide new candidates to T Tauri stars (TTSs) in the Taurus-Auriga region, using its ultraviolet excess as our baseline. The initial data set was defined from the GALEX all sky survey (AIS). The GALEX satellite ob[...]texto impreso
Las estrellas t tauri (ett) son estrellas pre-secuencia principal de baja masa con discos circundantes y campos magneticos complejos. El material ionizado de la parte interior del disco es conducido a traves de las lineas de campo magnetico y ac[...]texto impreso
Gómez de Castro, Ana Inés ; López-Santiago, Javier ; Sestito, Paola ; Rodrigo Gudiel, Víctor ; López Martínez, Fátima ; Castro Rubio, Elisa de ; Cornide, Manuel ; Yáñez, Javier | Springer | 2011-09The Gould Belt is the local superassociation of star formation. The age of the Belt is some few 10(7) yr, henceforth, its population is dominated by luminous young OB associations and low mass pre-main sequence stars. Attempts to unveil the low [...]texto impreso
Gómez de Castro, Ana Inés ; López Santiago, Javier ; López Martínez, Fátima ; Sánchez, Néstor ; Castro Rubio, Elisa de ; Cornide Castro-Piñeiro, Manuel | Wiley | 2015-06-01The Taurus-Aurigamolecular 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 dus[...]texto impreso
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[...]texto impreso
Gómez de Castro, Ana Inés ; Sestito, Paola ; Sánchez, Néstor ; López Martínez, Fátima ; Seijas, Juan ; Gómez, Maite ; Rodríguez, Pablo ; Quintana, Jose ; Ubierna, Marcos ; Muñoz, Jacinto | Elsevier | 2014The Imaging and Slitless Spectroscopy Instrument (ISSIS) will be flown as part of the science instrumentation in the World Space Observatory-Ultraviolet (WSO-UV). ISSIS will be the first UV imager to operate in a high Earth orbit from a 2 m clas[...]