Further Criteria for the Existence of Steady Line-Driven Winds

In Paper I, we showed that steady line-driven disk wind solutions can exist by using "simple" models that mimic the disk environment. Here I extend the concepts introduced in Paper I and discuss many details of the analysis of the steady/unsteady nature of 1D line-driven winds. This work confirms the results and conclusions of Paper I, and is thus consistent with the steady nature of the 1D streamline line-driven disk wind models of Murray and collaborators and the 2.5D line-driven disk wind models of Pereyra and collaborators. When including gas pressures effects, as is routinely done in time-dependent numerical models, I find that the spatial dependence of the nozzle function continues to play a key role in determining the steady/unsteady nature of supersonic line-driven wind solutions. I show here that the existence/nonexistence of local wind solutions can be proved through the nozzle function without integrating the equation of motion. This work sets a detailed framework with which we will analyze, in a following paper, more realistic models than the "simple" models of Paper I.Comment: 30 pages, 5 figures, accepted for publication by The Astrophysical Journa

Characterizing a CCD detector for astronomical purposes: OAUNI Project

This work verifies the instrumental characteristics of the CCD detector which is part of the UNI astronomical observatory. We measured the linearity of the CCD detector of the SBIG STXL6303E camera, along with the associated gain and readout noise. The linear response to the incident light of the detector is extremely linear (R2 =99.99%), its effective gain is 1.65 +/- 0.01 e-/ADU and its readout noise is 12.2 e-. These values are in agreement with the manufacturer. We confirm that this detector is extremely precise to make measurements for astronomical purposes.Comment: 6 pages, 8 figures, Published by TECNIA (UNI

La inclusión de la dimensión económica en la Evaluación de Impacto Ambiental

El objetivo de este trabajo es mostrar la importancia de incluir la dimensión económica en los Estudios deImpacto ambiental (EsIA). Dimensión económica que se incorpora a la evaluación “ex–ante” de inversiones a través del análisis beneficios costos (ABC) y la valoración económica de las externalidades (VEE). El trabajo muestra con ilustraciones y la presentación de dos casos las consecuencias no deseables de ignorar el ABC: a) Existencia de proyectos de eficiencia dudosa en términos de su resultado económico-social; y b) Escasez de proyectos ambientalmente eficientes, pero con escaso retorno económico privado

Proximal nested sampling with data-driven priors for physical scientists

Proximal nested sampling was introduced recently to open up Bayesian model selection for high-dimensional problems such as computational imaging. The framework is suitable for models with a log-convex likelihood, which are ubiquitous in the imaging sciences. The purpose of this article is two-fold. First, we review proximal nested sampling in a pedagogical manner in an attempt to elucidate the framework for physical scientists. Second, we show how proximal nested sampling can be extended in an empirical Bayes setting to support data-driven priors, such as deep neural networks learned from training data.Comment: 9 pages, 4 figure

Propósitos de una experiencia formativa con jóvenes : el sentido de las prácticas socioeducativas como vínculo entre educación y trabajo social

El objetivo de esta comunicación es reflexionar sobre nuestra propuesta de formación del curso Educación y Trabajo Social, analizando la integración de los saberes del campo de la pedagogía y del trabajo social, en torno a las prácticas socioeducativas como experiencia formativa. Analizaremos la configuración de la propuesta pedagógica centrándonos en la relación entre enseñanza, aprendizaje y prácticas socioeducativas, como eje de la formación para la intervención profesional. En esta reflexión consideramos a la Enseñanza como una práctica social, que se conforma a través de un proceso de interacción socio-histórica, cultural y política que promueve la formación. Por ello, proponemos la formación del/de la futuro/a profesional en trabajo social, incentivando la construcción de saberes en torno a la cuestión social vinculados con el ámbito socioeducativo, mediante el análisis de problemáticas comunitarias situadas, desde una perspectiva socio-pedagógica en función de la cual, orienta su práctica de intervención en la comunidad en el marco de programas institucionales de nuestra unidad académica.Fil: Pereyra, Sonia N.. Universidad Nacional de San Luis.Fil: Calderón, Marcela I.. Universidad Nacional de San Luis

Mental models for the negation of conjunctions and disjunctions

This study investigates why reasoning that involves negation is extremely difficult. We presented participants with reasoning problems containing sentences with negation of conjunctions and disjunctions in order to test predictions derived from the Mental Models Theory of human thought. According to this theory, reasoning consists of representing and comparing possibilities. Different sentential forms would require different cognitive demands. In particular, responses to a sentential negation task would be modulated by working memory load. This prediction would hold for correct responses but also for the general pattern of responses that includes incorrect responses when the task offers different response options. A within-subjects experimental design with selection paradigm was applied to test these predictions. Experimental comparisons and a complementary descriptive study yielded evidence consistent with the theory-driven predictions derived from the Mental Models Theory. The working memory load was critical for the modulation of correct responses and overall responses. We discussed alternative accounts, and suggested additional predictions for further evaluation of these phenomena

On the Steady Nature of Line-Driven Disk Winds

We perform an analytic investigation of the stability of line-driven disk winds, independent of hydrodynamic simulations. Our motive is to determine whether or not line-driven disk winds can account for the wide/broad UV resonance absorption lines seen in cataclysmic variables (CVs) and quasi-stellar objects (QSOs). In both CVs and QSOs observations generally indicate that the absorption arising in the outflowing winds has a steady velocity structure on time scales exceeding years (for CVs) and decades (for QSOs). However, published results from hydrodynamic simulations of line-driven disk winds are mixed, with some researchers claiming that the models are inherently unsteady, while other models produce steady winds. The analytic investigation presented here shows that if the accretion disk is steady, then the line-driven disk wind emanating from it can also be steady. In particular, we show that a gravitational force initially increasing along the wind streamline, which is characteristic of disk winds, does not imply an unsteady wind. The steady nature of line-driven disk winds is consistent with the 1D streamline disk-wind models of Murray and collaborators and the 2.5D time-dependent models of Pereyra and collaborators. This paper emphasizes the underlying physics behind the steady nature of line-driven disk winds using mathematically simple models that mimic the disk environmen

Characteristic QSO Accretion Disk Temperatures from Spectroscopic Continuum Variability

Using Sloan Digital Sky Survey (SDSS) quasar spectra taken at multiple epochs, we find that the composite flux density differences in the rest frame wavelength range 1300-6000 AA can be fit by a standard thermal accretion disk model where the accretion rate has changed from one epoch to the next (without considering additional continuum emission components). The fit to the composite residual has two free parameters: a normalizing constant and the average characteristic temperature $\bar{T}^*$. In turn the characteristic temperature is dependent on the ratio of the mass accretion rate to the square of the black hole mass. We therefore conclude that most of the UV/optical variability may be due to processes involving the disk, and thus that a significant fraction of the UV/optical spectrum may come directly from the disk.Comment: 31 pages, 8 figure

Control de especies de plata alojadas en zeolita A para la optimización de la adsorción por interacción Π

En las zeolitas intercambiadas con Ag+, la activación térmica o reducción química son metodologías para lograr la formación de nano-especies en la estructura del sólido. El proceso involucra la transferencia de carga desde el oxígeno, perteneciente a la red del sólido o al agente reductor químico, hacia el orbital 5s de los cationes Ag+. En este trabajo se estudiaron, mediante HRTEM y UV-vis, diferentes estrategias para el control de las propiedades de las especies de Ag estabilizadas en una zeolita A sintetizada en nuestro laboratorio

On the Steady Nature of Line-Driven Disk Winds: Application to Cataclysmic Variables

We apply the semi-analytical analysis of the steady nature of line-driven winds presented in two earlier papers to disk winds driven by the flux distribution of a standard Shakura & Sunyaev (1973) disk for typical cataclysmic variable (CV) parameters. We find that the wind critical point tends to be closer to the disk surface towards the inner disk regions. Our main conclusion, however, is that a line-driven wind, arising from a steady disk flux distribution of a standard Shakura-Sunyaev disk capable of locally supplying the corresponding mass flow, is steady. These results confirm the findings of an earlier paper that studied "simple" flux distributions that are more readily analyzable than those presented here. These results are consistent with the steady velocity nature of outflows observationally inferred for both CVs and quasi-stellar objects (QSOs). We find good agreement with the 2.5D CV disk wind models of Pereyra and collaborators. These results suggest that the likely scenario to account for the wind outflows commonly observed in CVs is the line-driven accretion disk wind scenario, as suggested early-on by Cordova & Mason (1982). For QSOs, these results show that the line-driven accretion disk wind continues to be a promising scenario to account for the outflows detected in broad absorption line (BAL) QSOs, as suggested early-on by Turnshek (1984), and analyzed in detail by Murray et al. (1995).Comment: 35 pages, 20 figure