12 resultados para UDK:656
em Consorci de Serveis Universitaris de Catalunya (CSUC), Spain
Resumo:
We present optical spectroscopy of MWC 656 and MWC 148, the proposed optical counterparts of the gamma-ray sources AGL J2241+4454 and HESS J0632+0 57, respectively. The main parameters of the Halpha emission line (EW, FWHM and centroid velocity) in these stars are modulated on the proposed orbital periods of 60.37 and 321 days, respectively. These modulations are likely produced by the resonant interaction of the Be discs with compact stars in eccentric orbits. We also present radial velocity curves of the optical stars folded on the above periods and obtain the first orbital elements of the two gamma-ray sources thus confirming their binary nature. Our orbital solution support eccentricities e~0.4 and 0.83+-0.08 for MWC 656 and MWC 148, respectively. Further, our orbital elements imply that the X-ray outbursts in HESS J0632+057/MWC 148 are delayed ~0.3 orbital phases after periastron passage, similarly to the case of LS I +61 303. In addition, the optical photometric light curve maxima in AGL J2241+4454/MWC 656 occur ~0.25 phases passed periastron, similar to what is seen in LS I +61 303. We also find that the orbital eccentricity is correlated with orbital period for the known gamma-ray binaries. This is explained by the fact that small stellar separations are required for the efficient triggering of VHE radiation. Another correlation between the EW of Halpha and orbital period is also observed, similarly to the case of Be/X-ray binaries. These correlations are useful to provide estimates of the key orbital parameters Porb and e from the Halpha line in future Be gamma-ray binary candidates.
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[spa]El testamento de este obispo dumiense resulta interesante porque pone de manifiesto una de las principales tensiones del cristianismo en la época postconstantiniana: el dilema que se planteaba al obispo a la hora de elegir entre ser, ante todo, un buen cristiano o anteponer los intereses económicos del obispado. La legislación conciliar y civil conservada indica que, aunque la principal preocupación episcopal era la adecuada gestión de las propiedades eclesiásticas, tampoco se olvidaron de practicar la caridad -manifestada a través de las tareas asistenciales-. Asimismo, este documento resulta útil para conocer la situación de los dependientes eclesiásticos en la Hispania del s. VII.
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Vegeu el resum a l'inici del document del fitxer adjunt
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We identify in this paper two conditions that characterize the domain of single-peaked preferences on the line in the following sense: a preference profile satisfies these two properties if and only if there exists a linear order $L$ over the set of alternatives such that these preferences are single-peaked with respect L. The first property states that for any subset of alternatives the set of alternatives considered as the worst by all agents cannot contains more than 2 elements. The second property states that two agents cannot disagree on the relative ranking of two alternatives with respect to a third alternative but agree on the (relative) ranking of a fourth one. Classification-JEL: D71, C78
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El projecte de fi de carrera proposat consisteix en l'anàlisi, disseny i implementació d'un conjunt de components que simplifiquen la construcció de la capa de presentació per a aplicacions web, servint de base per al desenvolupament d'altres productes.
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A version of Matheron’s discrete Gaussian model is applied to cell composition data.The examples are for map patterns of felsic metavolcanics in two different areas. Q-Qplots of the model for cell values representing proportion of 10 km x 10 km cell areaunderlain by this rock type are approximately linear, and the line of best fit can be usedto estimate the parameters of the model. It is also shown that felsic metavolcanics in theAbitibi area of the Canadian Shield can be modeled as a fractal
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This paper proposes to estimate the covariance matrix of stock returnsby an optimally weighted average of two existing estimators: the samplecovariance matrix and single-index covariance matrix. This method isgenerally known as shrinkage, and it is standard in decision theory andin empirical Bayesian statistics. Our shrinkage estimator can be seenas a way to account for extra-market covariance without having to specifyan arbitrary multi-factor structure. For NYSE and AMEX stock returns from1972 to 1995, it can be used to select portfolios with significantly lowerout-of-sample variance than a set of existing estimators, includingmulti-factor models.
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En el ámbito mediterráneo es frecuente la concurrencia en un mismo hábitat de especies perennifolias y caducifolias como Quercus ilex y Q. faginea. En este estudio se pretende analizar la diferencia en la respuesta ecofisiológica de las dos especies frente a la variación climática estacional mediante la composición isotópica de carbono de la materia orgánica soluble de las hojas (δ13Ch) y de la α-celulosa de la madera (δ13Cm). Se observaron patrones intraanuales dependientes de la especie en la δ13Ch. Por un lado, Q. faginea utiliza reservas de almidón como fuente de carbono para producir nuevas hojas a principios de abril, dando lugar a valores altos de δ13Ch. Por otro, Q. ilex utiliza asimilados recientes de las hojas formadas el año anterior (aún funcionales). No obstante, los valores globales de δ13Ch en ambas especies son similares (-25,4±0,55 y -25,5±0,89, para Q. faginea y Q. ilex, respectivamente), lo que apunta a valores equivalentes de eficiencia intrínseca en el uso del agua. Como en las hojas, la δ13Cm de Q. faginea reflejó claramente el uso de reservas en la madera temprana. Tanto la δ13Ch como la δ13Cm de las dos especies registran ajustes como respuesta a las variaciones ambientales estacionales. No obstante, y como parámetro integrador de eficiencia hídrica, la menor amplitud de las variaciones en la δ13Cm de Q. ilex sugiere una menor sensibilidad de esta especie frente a las fluctuaciones climáticas, lo que puede otorgarle cierta ventaja competitiva bajo condiciones de incremento progresivo de aridez.
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Stellar-mass black holes have all been discovered through X-ray emission, which arises from the accretion of gas from their binary companions (this gas is either stripped from low-mass stars or supplied as winds from massive ones). Binary evolution models also predict the existence of black holes accreting from the equatorial envelope of rapidly spinning Be-type stars (stars of the Be type are hot blue irregular variables showing characteristic spectral emission lines of hydrogen). Of the ~80 Be X-ray binaries known in the Galaxy, however, only pulsating neutron stars have been found as companions. A black hole was formally allowed as a solution for the companion to the Be star MWC 656 (also known as HD 215227), although that was based on a single radial velocity curve of the Be star, a mistaken spectral classification and rough estimates of the inclination angle. Here we report observations of an accretion disk line mirroring the orbit of the Be star. This, together with an improved radial velocity curve of the Be star through fitting sharp Fe II profiles from the equatorial disk, and a refined Be classification (to that of a B1.5-B2 III star), reveals a black hole of 3.8 to 6.9 solar masses orbiting MWC 656, the candidate counterpart of the gamma-ray source AGL J2241+4454. The black hole is X-ray quiescent and fed by a radiatively inefficient accretion flow giving a luminosity less than 1.6 x 10-7 times the Eddington luminosity. This implies that Be binaries with black-hole companions are difficult to detect by conventional X-ray surveys.
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The binding energies of deformed even-even nuclei have been analyzed within the framework of a recently proposed microscopic-macroscopic model. We have used the semiclassical Wigner-Kirkwood ̄h expansion up to fourth order, instead of the usual Strutinsky averaging scheme, to compute the shell corrections in a deformed Woods-Saxon potential including the spin-orbit contribution. For a large set of 561 even-even nuclei with Z 8 and N 8, we find an rms deviation from the experiment of 610 keV in binding energies, comparable to the one found for the same set of nuclei using the finite range droplet model of Moller and Nix (656 keV). As applications of our model, we explore its predictive power near the proton and neutron drip lines as well as in the superheavy mass region. Next, we systematically explore the fourth-order Wigner-Kirkwood corrections to the smooth part of the energy. It is found that the ratio of the fourth-order to the second-order corrections behaves in a very regular manner as a function of the asymmetry parameter I=(N−Z)/A. This allows us to absorb the fourth-order corrections into the second-order contributions to the binding energy, which enables us us to simplify and speed up the calculation of deformed nuclei.
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Background Exhausting exercise reduces the mitochondrial DNA (mtDNA) content in the skeletal muscle of healthy subjects due to oxidative damage. Since patients with chronic obstructive pulmonary disease (COPD) suffer enhanced oxidative stress during exercise, it was hypothesised that the mtDNA content will be further reduced. Objective To investigate the effects of exercise above and below the lactate threshold (LT) on the mtDNA content of skeletal muscle of patients with COPD. Methods Eleven patients with COPD (676 8 years; forced expiratory volume in 1s (FEV1)456 8%ref) and 10 healthy controls (666 4 years; FEV1 906 7% ref) cycled 45 min above LT (65% peak oxygen uptake (V9O2 peak)and another 7 patients (656 6 years; FEV1 506 4%ref)and 7 controls (566 9 years;FEV1 926 6%ref) cycled 45 min below their LT (50% V9O2 peak). Biopsies from the vastus lateralis muscle were obtained before exercise, immediately after and 1 h, 1 day and 1 week later to determine by PCR the mtDNA/nuclear DNA (nDNA) ratio (a marker of mtDNA content) and the expression of the peroxisome proliferator-activated receptor- g coactivator-1 a (PGC-1a)mRNA and the amount of reactive oxygen species produced during exercise was estimated from total V9O2. Results Skeletal muscle mtDNA/nDNA fell significantly after exercise above the LT both in controls and in patients with COPD, but the changes were greater in those with COPD. These changes correlated with production of reactive oxygen species, increases in manganese superoxide dismutase and PGC-1 a mRNA and returned to baseline values 1 week later. This pattern of response wa was also observed, albeit minimised, in patients exercising below the LT. Conclusions In patients with COPD, exercise enhances the decrease in mtDNA content of skeletal muscle and the expression of PGC-1 a mRNA seen in healthy subjects probably due to oxidative stress.
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Several studies have linked coping with personal wellbeing. However, there is no research evidence analyzing this relationship in theSpanish population using Cummins’ model (1997). The aim of this study was to know the level of personal wellbeing of a sample of adolescents and to analyze the relationship between coping strategies and styles and personal well-being. With that purpose in mind, the Personal Well Being Index (PWI) and the Adolescent Coping Scale (ACS) have been administered to a sample of 656 adolescents aged between 11 and 17. The results allow identifying the effect of age and gender on personal wellbeing. Those coping strategies centered on focusing on the positive, physical recreation, working hard and achieving are associated to higher personal wellbeing while self-blaming and keeping to self are with lower personal wellbeing