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Betoré, M. Pilar ; Casado González, Miguel Ángel ; García Orduña, Pilar ; Lahoz, Fernando J. ; Polo, Víctor ; Oro, Luis A. | Wiley-VCH Verlag GmbH | 2016-07The treatment of [(Ir(?-Cl)(cod))2] (cod = 1,5-cyclooctadiene) with 2,5-norbornadiene (nbd) in the presence of triethylphosphane under an atmosphere of ammonia afforded the cation complex [Ir(?C,?C-C21H24)(NH3)3(PEt3)]Cl (1a) and complex [Ir(?C,[...]texto impreso
We establish a formula for the measure of non-compactness of an operator interpolated by the general real method generated by a sequence lattice ?. The formula is given in terms of the norms of the shift operators in ?.texto impreso
Caballero, J. A. ; Cornide Castro-Piñeiro, Manuel ; Castro Rubio, Elisa de | Wiley-VCH Verlag GmbH | 2010-03We look for high-amplitude variable young stars in the open clusters and associations of the Orion Belt. We use public data from the ASAS-3 Photometric V -band Catalogue of the All Sky Automated Survey, infrared photometry from the 2MASS and IRA[...]texto impreso
López Dolado, Elisa ; González Mayorga, Ankor ; Portoles, María Teresa ; Feito Castellano, María José ; Ferrer, María Luisa ; Monte, Francisco del ; Gutiérrez, María Concepción ; Serrano, María Concepción | Wiley-VCH Verlag GmbH | 2015The increasing prevalence and high sanitary costs of lesions affecting the central nervous system (CNS) at the spinal cord are encouraging experts in different fields to explore new avenues for neural repair. In this context, graphene and its de[...]texto impreso
Villaverde, Gonzalo ; Gómez-Graña, Sergio ; Guisasola, Eduardo ; García, Isabel ; Hanske, Cristoph ; Liz-Marzan, Luis M ; Baeza, Alejandro ; Vallet Regí, María | Wiley-VCH Verlag GmbH | 2018Melanoma is one of the most severe public health issues worldwide, not onlybecause of the high number of cases but also for its poor prognosis in late stages. Therefore, early diagnosis and efficient treatment are key toward a future solution. H[...]texto impreso
Luminosity functions are one of the most important observational clues when studying galaxy evolution over cosmic time. In this paper we present the X-ray luminosity functions for X-ray detected AGN in the SXDS and GWS fields. The limiting fluxe[...]
