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La sociedad, como ente dinámico, sufre variaciones a nivel cultural, social, económico o político y la atención sanitaria debe adaptarse a éstas, satisfaciendo las nuevas necesidades que van surgiendo. El objetivo de la investigación es analizar las necesidades sociosanitarias que presenta la población en la actualidad y determinar si es necesario incluir nuevos contenidos curriculares en el futuro Grado de Enfermería de la Universidad de Valladolid, para dar respuesta a las mismas. Se analizarán los aspectos claves que conforman el contexto sociosanitario. Así, se estudiará el perfil demográfico de la sociedad española, el progresivo envejecimiento poblacional, la atención a las personas dependientes, el estado de salud de la población, la violencia de género, la interrupción voluntaria del embarazo y la salud sexual y reproductiva, l...
Inorganic polyphosphate (poly P) is a polymer made from as few as 10 to several hundred phosphate molecules linked by phosphoanhydride bonds similar to ATP. Poly P is ubiquitous in all mammalian organisms, where it plays multiple physiological roles. The metabolism of poly P in mammalian organisms is not well understood. We have examined the mechanism of poly P production and the role of this polymer in cell energy metabolism. Poly P levels in mitochondria and intact cells were estimated using a fluorescent molecular probe, 4',6-diamidino-2-phenylindole. Poly P levels were dependent on the metabolic state of the mitochondria. Poly P levels were increased by substrates of respiration and in turn reduced by mitochondrial inhibitor(rotenone) or an uncoupler(carbonyl cyanide p-trifluoromethoxyphenylhydrazone). Oligomycin, an inhibitor of m...
We present a compilation of spectroscopic observations of the sgB[e] star CI Cam, the optical counterpart of XTE J0421+560. This includes data from before, during, and after its 1998 outburst, with quantitative results spanning 37 years. The object shows a rich emission line spectrum originating from circumstellar material, rendering it difficult to determine the nature of either star involved or the cause of the outburst. We collate all available pre-outburst data to determine the state of the system before this occurred and provide a baseline for comparison with outburst and post-outburst data. During the outburst all lines become stronger, and hydrogen and helium lines become significantly broader and asymmetric. After the outburst, spectral changes persist for at least three years, with Fe II and [N II] lines still a factor of simi...