bluuebunny/crossref_metadata_2025_split huggingface dataset:
Violencia contra la mujer y regulación jurídica del femicidio en Ecuador
Authors: Goyas Cespedes Lianet , Zambrano Noles Silvia Patricia , Cabanes Espino Iris 
Published: October 2018

<p>La violencia contra las mujeres es reconocida como un problema social a nivel mundial, aunque es difícil de expresar en cifras por la cantidad de casos que no son denunciados; según datos de la Encuesta Nacional sobre Relaciones Familiares y Violencia de Género, en Ecuador la violencia por razón de género ha afectado a seis de cada diez mujeres. Ante esta situación, la sociedad civil y los gobiernos trazan estrategias para la erradicación de todas las formas de violencia contra la mujer, entre las que se encuentra la tipificación del femicidio en las legislaciones de varios países latinoamericanos, pero esto no ha parado las muertes de mujeres por razón de su género. Todo esto motiva el análisis de la regulación en varios países de América Latina respecto a la figura del femicidio, con especial referencia en Ecuador, que se presenta en este artículo como resultado del proyecto de investigación “Deberes y derechos ciudadanos”, que se desarrolla en la Universidad Metropolitana del Ecuador.</p>
El derecho de los adultos mayores a la seguridad social y la pensión de vejez reducida
Authors: Martínez Martínez Verónica Lidia 
Published: October 2018

<p>Partiendo de los ordenamientos que fundamentan el derecho de los adultos mayores a la seguridad social en el sistema jurídico mexicano, así como de la forma de acceder al seguro de vejez, en el presente trabajo se expone el incumplimiento al convenio (número 102) sobre la seguridad social (norma mínima), ante la inexistencia de la pensión reducida de vejez en la Ley del Seguro Social. Fundamental fue el análisis de las disposiciones normativas nacionales e internacionales aplicables en el caso de México a los adultos mayores y, en especial, los ordenamientos que reglamentan el derecho a la pensión de vejez. Desde el punto de vista metodológico, la investigación requirió de la consulta de fuentes especializadas en Derecho Constitucional, Derecho Internacional de los Derechos Humanos y Seguridad Social, que, en comunión con los métodos analítico y deductivo, nos permitieron comprender el tipo de prestaciones que resultan procedentes en el seguro de vejez, los requisitos para acceder a ellas<br />y la inobservancia al convenio número 102 como norma internacional de derechos humanos.</p>
La violación de derechos humanos en la Ley de Instituciones de Crédito
Authors: Jiménez González Víctor Hugo 
Published: October 2018

<p>En México, el ordenamiento jurídico financiero regulador de las prácticas bancarias, específicamente el artículo 100 de la Ley de Instituciones de Crédito, pareciera quedar fuera del alcance de las normas constitucionales garantes de los derechos humanos de seguridad e igualdad jurídica y de acceso a una justicia imparcial en la que se cumplan las formalidades esenciales del procedimiento, toda vez que el artículo al que se hace referencia contempla, en caso de controversia, la posibilidad de que las instituciones bancarias, en beneficio de sus intereses, puedan aportar como medio de prueba impresiones certificadas por funcionario autorizado por ellas mismas, las cuales tendrán en juicio el mismo valor probatorio que libros, registros y documentos microfilmados o grabados en discos ópticos obtenidos de sus originales. Tal disposición sitúa en indefensión legal al cuentahabiente dado que a la institución de crédito le es permisible, de cierta manera, la potencial manufactura de sus medios probatorios.</p>
La ideología en el Derecho y una sentencia uruguaya acerca del IVA
Authors: Blanco Andrés Javier 
Published: October 2018

<p>El análisis ideológico del discurso del Derecho es una de las vertientes más originales de la Teoría del Derecho en tanto apunta a conectar los contenidos de la legislación, la dogmática y la jurisprudencia con fenómenos sociales reales en términos funcionales. En el presente trabajo, luego de proponer un marco teórico del análisis ideológico, se presenta un caso real de la jurisprudencia uruguaya sobre el Impuesto al Valor Agregado (IVA), en el cual el análisis ideológico de la sentencia ilumina su sentido.</p>
El concepto de libertad en Hannah Arendt para el ejercicio de los derechos humanos
Authors: Delgado Parra Ma. Concepción 
Published: October 2018

<p>El concepto de libertad en la obra de Hannah Arendt constituye un elemento fundamental para actualizar la reflexión y el ejercicio de los derechos humanos en el contexto presente. Su propuesta radica en colocar la acción política en el centro de la libertad para pensar el vínculo entre la ley y su puesta en marcha para realizar los derechos humanos. Con este propósito, argumenta sobre los límites que entraña el principio de que los derechos humanos tienen su concreción en el marco de un sistema estatal soberano, ratificado en todas las declaraciones universales desde la Revolución francesa. Al mismo tiempo, postula la concepción del “derecho a tener derechos” como una alternativa que pone en relación el derecho moral a “ser miembro”, con el derecho político de “actuar en la pluralidad y emitir juicios” al interior de una comunidad política.</p>
Gobernanza y desarrollo local: estudio para la junta auxiliar de San Baltazar Tetela, en el municipio de Puebla, Puebla
Authors: Miquel Hernández Montserrat , Cazarín Martínez Angélica 
Published: October 2018

<p>El objetivo de este artículo es analizar los procesos de gobernanza territorial en la comunidad de San Baltazar Tetela, en el municipio de Puebla, a través de lo que las autoridades establecen como su principal fuente de ingresos: la panga Mónica II. En este contexto, es importante destacar que la base teórica que sustenta el trabajo es el desarrollo local, entendido como un proceso sociopolítico donde la articulación de actores tiene un papel central para la gestión local y la gobernanza territorial, la cual establece la inclusión de los actores comunitarios que, a través de su identidad con el territorio, hacen que la toma de decisiones presente un estándar mayor de legitimidad y aceptación. Para ello, se hace una revisión documental respecto a la junta auxiliar, así como entrevistas de profundidad con los principales actores involucrados en la panga, donde se resalta que la ausencia de un liderazgo conlleva a la falta de consenso acerca del futuro del proyecto local turístico como fuente de ingresos y empleos en beneficio de los habitantes de la comunidad. </p>
Tres críticas de Heidegger a las bases de la fenomenología de Husserl
Authors: Sánchez-Soberano Ramsés 
Published: October 2018

<p align="justify">La finalidad de este trabajo es la elucidación de los problemas de la interpretación heideggeriana que pone en relación el hombre, la lógica y la verdad y que han dado pauta a más de un pensar actual. Hemos utilizado la primera edición de las <em>Logische Untersuchungen</em> para adecuarnos a los análisis husserlianos primitivos y, paralelamente, a la lectura que Heidegger realizó de aquel texto y que anunció en más de una ocasión. Con ello, podremos vislumbrar que la lógica y la ontología luchan por colocarse como la ciencia más originaria para la elucidación final del ser. Así, nos preparamos para tomar una posición definitiva frente a la convicción actual que acepta de suyo que el teoreticismo husserliano ha sido superado por el planteamiento pragmático del <em>Dasein</em>.</p>
GOLD AND MERCURY IN THE PROCESSES OF ORE FORMATION IN KAMCHATKA
Authors: STEPANOV V. A. 
Published: October 2018

The main features of the difference and similarity of the physical and chemical properties of gold and mercury have been given, which determine their behavior in the natural processes of formation of deposits of both metals in Kamchatka. It has been shown that the difference in the properties of gold and mercury led to the emergence of independent monometallic deposits, differing in connection with intrusive formations, in depth and temperature of ore formation. The similarity of the properties of these elements determined the appearance of mercury minerals on gold ore deposits and gold in mercury deposits, as well as the formation of complex gold-mercury deposits. Four geological-industrial types of gold- mercury deposits have been distinguished: the Knoxville, the Carlin, the Kyuchus and the Chemlian ones, which include deposits with large gold reserves both abroad and in Russia. The identification of gold deposits, including through the revision of mercury ore occurrences and deposits of Kamchatka for gold presence, will strengthen the mineral resources base of gold in this region.
El discurso de la muerte en la cuentística de El caballero Carmelo de Abraham Valdelomar. Aproximaciones narratológicas
Authors: Hernández Luis Morón 
Published: October 2018

Dentro de los trabajos interpretativos de los cuentos de Valdelomar no suele estudiarse el tópico de la muerte en los cuentos del Caballero Carmelo. Este trabajo intenta realizar una aproximación narratológica y establecer la relación entre el discurso de la muerte y los principales cuentos del genial narrador iqueño. El Caballero Carmelo (CC en adelante), libro de cuentos publicado en 1918 con el título: El Caballero Carmelo. Cuentos de Abraham Valdelomar con un prólogo de D. Alberto Ulloa Sotomayor y un apéndice crítico sobre esta y otras obras del artista, comprende varios cuentos integrados ; inicialmente con el cuento que lleva el título del libro y secundado por otros conocidos como: El vuelo de los cóndores, Hebaristo, el sauce que murió de amor, Los ojos de Judas, Yerba Santa, Tres senas; dos ases, El beso de Evans, El círculo de la muerte, Finis desolatrix veritae, Chaymanta huayñuy, entre otros, que comprende dieciséis cuentos, muchos de ellos publicados por décadas en diversas antologías.
Constraining Stellar-mass Black Hole Mergers in AGN Disks Detectable with LIGO
Authors: McKernan Barry , Saavik Ford K. E. , Bellovary J. , Leigh N. W. C. , Haiman Z. , Kocsis B. , Lyra W. , Mac Low M.-M. , Metzger B. , O’Dowd M. , Endlich S. , Rosen D. J. 
Published: October 2018

Abstract
Black hole (BH) mergers detectable with the Laser Interferometer Gravitational-wave Observatory (LIGO) can occur in active galactic nucleus (AGN) disks. Here we parameterize the merger rates, the mass spectrum, and the spin spectrum of BHs in AGN disks. The predicted merger rate spans ∼10−3–104 Gpc−1 yr−1, so upper limits from LIGO (<212 Gpc−1 yr−1) already constrain it. The predicted mass spectrum has the form of a broken power law, consisting of a pre-existing BH power-law mass spectrum and a harder power-law mass spectrum resulting from mergers. The predicted spin spectrum is multipeaked with the evolution of retrograde spin BHs in the gas disk playing a key role. We outline the large uncertainties in each of these LIGO observables for this channel and we discuss ways in which they can be constrained in the future.
Theoretical Model of Hydrogen Line Emission from Accreting Gas Giants
Authors: Aoyama Yuhiko , Ikoma Masahiro , Tanigawa Takayuki 
Published: October 2018

Abstract
Progress in understanding of giant planet formation has been hampered by a lack of observational constraints to growing protoplanets. Recently, detection of an Hα-emission excess via direct imaging was reported for the protoplanet LkCa15b orbiting the pre-main-sequence star LkCa15. However, the physical mechanism for the Hα emission is poorly understood. According to recent high-resolution three-dimensional hydrodynamic simulations of the flow accreting onto protoplanets, the disk gas flows down almost vertically onto and collides with the surface of a circumplanetary disk at a supersonic velocity and thus passes through a strong shockwave. The shock-heated gas is hot enough to generate Hα emission. Here we develop a one-dimensional radiative hydrodynamic model of the flow after the shock by detailed calculations of chemical reactions and electron transitions in hydrogen atoms, and quantify the hydrogen line emission in the Lyman-, Balmer-, and Paschen-series from the accreting gas giant system. We then demonstrate that the Hα intensity is strong enough to be detected with current observational techniques. Comparing our theoretical Hα intensity with the observed one from LkCa15b, we constrain the protoplanet mass and the disk gas density. Observation of hydrogen line emission from protoplanets is highly encouraged to obtain direct constraints of accreting gas giants, which will be key in understanding the formation of gas giants.
Independent Estimation of Black Hole Mass for the γ-ray-detected Archetypal Narrow-line Seyfert 1 Galaxy 1H 0323+342 from X-Ray Variability
Authors: Pan Hai-Wu , Yuan Weimin , Yao Su , Komossa S. , Jin Chichuan 
Published: October 2018

Abstract

γ-ray-detected narrow-line Seyfert 1 galaxies (NLS1s) are a newly discovered class of radio-loud active galactic nuclei (AGNs) that launch powerful jets that are generally found only in blazars and radio galaxies. However, their black hole (BH) masses as estimated from their broad emission lines are an order of magnitude or more lower than those in blazars. This poses new challenges in explaining the triggering of radio loudness in AGNs. It is still under debate whether their BH masses are underestimated by the commonly used virial method. Here we present an estimate of the BH mass for the γ-ray-detected NLS1 1H 0323+342, an archetype of this class, from its X-ray variability, which is independent of inclination. Our results independently confirm that this NLS1 harbors a

BH similar to those in normal NLS1s rather than those in blazars.
Stellar and AGN Feedback in Isolated Early-type Galaxies: The Role in Regulating Star Formation and ISM Properties
Authors: Li Ya-Ping , Yuan Feng , Mo Houjun , Yoon Doosoo , Gan Zhaoming , Ho Luis C. , Wang Bo , Ostriker Jeremiah P. , Ciotti Luca 
Published: October 2018

Abstract
How galaxies maintain the inefficiency of star formation with physically self-consistent models is a central problem in understanding galaxy evolution. Although numerous theoretical models have been proposed in recent decades, the debate continues. By means of high-resolution two-dimensional hydrodynamical simulations, we study the three feedback effects (the stellar wind heating, supernova (SN) feedback, and active galactic nucleus (AGN) feedback) in suppressing star formation activities on the evolution of early-type galaxies with different stellar masses. The AGN feedback models are updated from work by Yuan et al. The gas sources arise exclusively from the mass losses of dying low-mass stars for most of our models. We find that SN feedback can keep star formation at a significantly low level for low-mass elliptical galaxies for a cosmological evolution time. For high-mass galaxies, AGN feedback can efficiently offset radiative cooling and thus regulate star formation activity. Such a suppression of star formation is extremely efficient in the inner regions of galaxies. Asymptotic giant branch heating cannot account for this suppression for low- or high-mass galaxies. The X-ray temperature T
X and luminosity L
X of hot plasma can be in agreement with the observed data with the inclusion of effective feedback processes. These results thus suggest that we can use T
X and L
X to probe the role of different feedback processes. The inclusion of additional gas sources can cause the mass scale between SN and AGN feedback to dominate in suppressing star formation decrease to an observationally inferred value of a few 1010 M
⊙.
Widespread Shocks in the Nucleus of NGC 404 Revealed by Near-infrared Integral Field Spectroscopy
Authors: Boehle A. , Larkin J. E. , Armus L. , Wright S. A. 
Published: October 2018

Abstract
We present high spatial resolution, integral field spectrograph (IFS) observations of the nearby low-ionization nuclear emission-line region (LINER) galaxy NGC 404 at 1.25 μm (J band) and 2.2 μm (K band) near-infrared (NIR) wavelengths. Although NGC 404 is thought to host an intermediate-mass black hole (BH) at its center, it has been unclear whether accretion onto the BH or another mechanism such as shock excitation drives its LINER emission at optical/NIR wavelengths. We use the OSIRIS IFS at Keck Observatory behind laser guide star adaptive optics to map the strength and kinematics of [Fe ii], H2, and hydrogen recombination lines at spatial resolutions of 1 pc across the central 30 pc of the galaxy. The H2 gas is in a central rotating disk, and ratios of multiple H2 lines indicate that the molecular gas is thermally excited, with some contribution from UV fluorescence. The [Fe ii] emission is more extended and diffuse than the molecular gas and has a different kinematic structure that reaches higher velocities/dispersions. We also map the strength of the CO stellar absorption feature and constrain the dominant age of the nuclear stellar population to ∼1 Gyr. Finally, we find regions across the nucleus of NGC 404 with [Fe ii]/Paβ line ratios up to 6.5, ∼2.5 times higher than the ratio measured from spatially integrated spectra. From these high line ratios, we conclude that shocks are the dominant physical mechanism exciting NGC 404's LINER emission and argue that a possible source of this shock excitation is a supernova remnant.
YZiCS: Preprocessing of Dark Halos in the Hydrodynamic Zoom-in Simulation of Clusters
Authors: Han San , Smith Rory , Choi Hoseung , Cortese Luca , Catinella Barbara , Contini Emanuele , Yi Sukyoung K. 
Published: October 2018

Abstract
To understand the galaxy population in clusters today, we should also consider the impact of previous environments prior to cluster infall, namely preprocessing. We use the Yonsei Zoom-in Cluster Simulation, a hydrodynamic high-resolution zoom-in simulation of 15 clusters, and focus on the tidal stripping suffered by the dark matter halos of cluster members due to preprocessing. We find that ∼48% of today’s cluster members were once satellites of other hosts. This is slightly higher than previous estimates, in part because we consider not just group-mass hosts but hosts of all masses. Thus, we find that the preprocessed fraction is poorly correlated with cluster mass and is instead related to each cluster’s recent mass growth rate. Hosts less massive than groups are significant contributors, providing more than one-third of the total preprocessed fraction. We find that halo mass loss is a clear function of the time spent in hosts. However, two factors can increase the mass-loss rate considerably: the mass ratio of a satellite to its host and the cosmological epoch when the satellite was hosted. The latter means we may have previously underestimated the role of high-redshift groups. From a sample of heavily tidally stripped members in clusters today, nearly three-quarters were previously in a host. Thus, visibly disturbed cluster members are more likely to have experienced preprocessing. Being hosted before cluster infall enables cluster members to experience tidal stripping for extended durations compared to direct cluster infall and at earlier epochs when hosts were more destructive.
Evolution of Quasar Stochastic Variability along Its Main Sequence
Authors: Sun Mouyuan , Xue Yongquan , Wang Junxian , Cai Zhenyi , Guo Hengxiao 
Published: October 2018

Abstract
We explore the evolution of the time variability (in the optical g-band and on timescales of weeks to years) of Sloan Digital Sky Survey Stripe 82 quasars along the quasar main sequence. A parent sample of 1004 quasars within 0.5 ≤ z ≤ 0.89 was used for our statistical studies; we then made subsamples from our parent sample: a subsample of 246 quasars with similar luminosities, and a subsample of 399 quasars with similar

(i.e., the ratio of the equivalent width of Fe ii within 4435–4685 Å to that of Hβ). We find the variability amplitude decreases with luminosity (L
bol). The anticorrelation between the variability amplitude and

is weak but statistically significant. The characteristic timescale, τ, correlates mostly with quasar luminosity; its dependence on

is statistically insignificant. After controlling luminosity and

, the high- and low-FWHM samples have similar structure functions. These results support the framework that

is governed by Eddington ratio and the FWHM of Hβ is mostly determined by orientation. We then provide new empirical relations between variability parameters and quasar properties (i.e., luminosity and

). Our new relations are consistent with the scenario that quasar variability is driven by thermal fluctuations in the accretion disk; τ seems to correspond to the thermal timescale. From our new relations, we find that the short-term variability is mostly sensitive to L
bol. Based on this we propose that quasar short-term (a few months) variability might be a new type of “Standard Candle” and can be adopted to probe cosmology.
Detectability of Double White Dwarfs in the Local Group with LISA
Authors: Korol Valeria , Koop Orlin , Rossi Elena M. 
Published: October 2018

Abstract
Detached double white dwarf (DWD) binaries are one of the main science cases for the Laser Interferometer Space Antenna (LISA). As the most numerous LISA sources, they will provide important contributions toward understanding binary evolution, supernovae Type Ia (SNIa) formation channels, and the structure of the Milky Way. So far only detection prospects for the Milky Way have been predicted. In this Letter we show that LISA has the potential to detect DWDs in neighboring galaxies up to the border of the Local Group. In particular, we compute quantitative estimates for the number of detections in M31. We expect between a dozen to several tens of DWDs above the nominal detection threshold, for a mission duration between 4 and 10 years. We show that detectable extra-galactic DWDs include those with the shortest orbital periods (P < 10 minutes) and with the highest chirp masses (

). This subgroup represents candidates for SNIa progenitors. These binaries are virtually undetectable at those distances in optical, implying that LISA could be the best instrument able to provide SNIa merger rates across the Local Group.
Simultaneous VLBI Astrometry of H2O and SiO Masers toward the Semiregular Variable R Crateris
Authors: Kim Dong-Jin , Cho Se-Hyung , Yun Youngjoo , Kyung Choi Yoon , Yoon Dong-Hwan , Kim Jaeheon , Dodson Richard , Rioja María J. , Yang Haneul , Yoon Suk-Jin 
Published: October 2018

Abstract
We obtained, for the first time, astrometrically registered maps of the 22.2 GHz H2O and 42.8, 43.1, and 86.2 GHz SiO maser emission toward the semiregular b-type variable (SRb) R Crateris, at three epochs (2015 May 21, and 2016 January 7 and 26) using the Korean Very-long-baseline Interferometry Network. The SiO masers show a ring-like spatial structure, while the H2O maser shows a very asymmetric one-side outflow structure, which is located at the southern part of the ring-like SiO maser feature. We also found that the 86.2 GHz SiO maser spots are distributed in an inner region, compared to those of the 43.1 GHz SiO maser, which is different from all previously known distributions of the 86.2 GHz SiO masers in variable stars. The different distribution of the 86.2 GHz SiO maser seems to be related to the complex dynamics caused by the overtone pulsation mode of the SRb R Crateris. Furthermore, we estimated the position of the central star based on the ring fitting of the SiO masers, which is essential for interpreting the morphology and kinematics of a circumstellar envelope. The estimated stellar coordinate corresponds well to the position measured by Gaia.