RT Journal Article
T1 The ultraviolet survey of the Gould Belt: general properties of the Taurus star forming region
A1 Gómez De Castro, Ana Inés
A1 López Santiago, Javier
A1 Sestito, Paola
A1 Rodrigo Gudiel, Víctor
A1 López Martínez, Fátima
A1 Castro Rubio, Elisa De
A1 Cornide, Manuel
A1 Yáñez, Javier
AB The 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 mass population have been run making use of the ROSAT all-sky survey. The all sky ultraviolet survey run by the GALaxy Evolution eXplorer (GALEX) maps several regions in the Belt. In this contribution, we present the preliminary analysis of the UV stellar population towards the Taurus region, one of the nearest and best studied regions of star formation.
PB Springer
SN 0004-640X
YR 2011
FD 2011-09
LK https://hdl.handle.net/20.500.14352/42236
UL https://hdl.handle.net/20.500.14352/42236
LA eng
NO Gómez de Castro, A. I., López Santiago, J., Sestito, P. et al. «The Ultraviolet Survey of the Gould Belt: General Properties of the Taurus Star Forming Region». Astrophysics and Space Science, vol. 335, n.o 1, septiembre de 2011, pp. 97-103. DOI.org (Crossref), https://doi.org/10.1007/s10509-011-0687-9.
NO Ministerio de Ciencia e Innovación
DS Docta Complutense
RD 4 abr 2025