bluuebunny/crossref_metadata_2025_split huggingface dataset:
HOMENAJE IN MEMORIAM AL DR. JORGE CARPIZO* JORGE CARPIZO, UN PRÓCER SIN OCASO
Authors: Valadés Diego 
Published: August 2018

<p> </p><p><span> </span><span>E</span>l 30 de marzo falleció Jorge Carpizo, figura señera del pensamiento jurídico mexicano. En el sentido más estricto del término fue un auténtico prócer. El trayecto de su vida fue de una coherencia ejemplar; nunca transigió con sus principios ni perdió la claridad de sus objetivos. Nació en Campeche el 2 de abril de 1944, y con toda justicia se le considera uno de los campechanos más importantes del siglo; siempre se sintió orgulloso de su oriundez.</p><p>Es difícil sintetizar la prolífica obra de Jorge Carpizo. Aun así, pese a su frialdad los números dicen mucho: 17 libros como autor único, 4 más como coautor y 16 coordinados; más de un centenar de ensayos en obras colectivas y revistas especializadas; casi una centena de prólogos; entre conferencias, discursos e intervenciones académicas superó las cuatro centenas; cerca de 30 tesis dirigidas y 154 congresos y seminarios, entre los organizados por él y a los que asistió, en su mayoría de carácter internacional.</p>
UNA APROXIMACIÓN CONCEPTUAL AL CONTROL JURISDICCIONAL DE CONSTITUCIONALIDAD
Authors: Brito Melgararejo Rodrigo 
Published: August 2018

<p> </p><p><span> </span>Este artículo tiene como fin ofrecer un marco teórico para el análisis de los principales elementos del concepto de control jurisdiccional de constitucionalidad. A través del examen de términos como <em>constitucionalidad</em>, <em>jurisdicción </em>y <em>control</em>, el autor propone una serie de reflexiones sobre la importancia de un estudio teórico de este mecanismo para determinar la constitucionalidad de leyes y actos de autoridad.</p>
EL DEBATE "HART-DWORKIN": UNA INTRODUCCIÓN A LA DISCUSIÓN
Authors: Gonzalez Covarrubias Maria De la Luz , Aspe de la Rosa Miguel Angel 
Published: August 2018

<p> El siglo pasado la historia</p><p>del conocimiento humano se nutrió con las</p><p>aportaciones de filósofos analíticos revolu<span> cionarios</span></p><p>intelectualmente como Ludwig</p><p>Wittgenstein particularmente con su meto<span>dología</span></p><p>de análisis del lenguaje. Su influencia</p><p>permea en filósofos del derecho generando</p><p>teorías jurídicas como la de H.L.A.</p><p>Hart y esta teoría a su vez se convierte en</p><p> punto de partida para otras explicaciones</p><p>como la de Ronald Dworkin, confirmándose</p><p> lo que Hart señalaba a propósito de la per<span>plejidad</span></p><p>que subyace en torno a la reflexión</p><p> sobre ¿qué es derecho? En este sentido, este</p><p>ensayo tiene como propósito identificar el</p><p> núcleo central alrededor del cual el debate</p><p>Hart-Dworkin está estructurado a manera de</p><p> introducción para los estudiantes y el lector</p><p>interesado.</p>
LAS NUEVAS TENDENCIAS SOBRE LA EJECUCIÓN PENAL
Authors: Mendoza Bremauntz Emma 
Published: August 2018

<p> Hay una preocupación real acerca de la manera cómo ha sido dirigida la ejecución penal desde el comienzo del siglo, especialmente, después del reconocimiento de los problemas que en la realidad se han desarrollado en las prisiones, instituciones que se utilizan para solucionar todos los problemas delictivos sin éxito. Las Naciones Unidas han propuesto algunas formas de regular y controlar estos problemas, pero muchas naciones miembros de la Organización no siguen sus resoluciones y no las toman en cuenta o no atienden el respeto a los derechos de los prisioneros. Necesitamos conocer, recordar y cumplir con nuestros compromisos internacionales para avanzar en el trato humano a los presos, recobrando la ruta humanitaria y actual.</p>
PRISIÓN PREVENTIVA Y REPARACIÓN DEL DAÑO EN MÉXICO: LEY GENERAL DE VÍCTIMAS Y FEDERAL DE RESPONSABILIDAD PATRIMONIAL DEL ESTADO
Authors: Mosri Gutiérrez Zulema 
Published: August 2018

<p>A partir de las recientes reformas en materia responsabilidad del Estado, derechos humanos y la transformación del sistema penal, se ha generado un debate respecto a la figura de la prisión preventiva injusta y sus mecanismos de reparación del daño. El sistema jurídico mexicano reconoce al menos dos esquemas para responder por los daños causados a las personas por la actuación estatal, los cuales, por su naturaleza, responden a supuestos distintos y están regulados en disposición también diferentes: la Ley General de Víctimas y la Ley Federal de Responsabilidad Patrimonial del Estado.</p>
LA VIOLACIÓN DEL DERECHO AL REFERENDO REVOCATORIO PRESIDENCIAL EN VENEZUELA
Authors: Hernández G. José Ignacio 
Published: August 2018

<p>En 2016 el Consejo Nacional Electoral, de manera arbitraria,<br />limitó el derecho ciudadano a solicitar el referendo revocatorio del mandato presidencial, como componente esencial de la democracia constitucional. Como consecuencia de ello, se impidió la realización de ese referendo en 2016, afectando así la solución constitucional a la grave crisis política venezolana.</p>
Marco Jurídico para Resguardar la Probidad en la Función Pública en Chile
Authors: Camacho Cepeda Gladys 
Published: August 2018

<p>En el presente artículo se plantea el diseño institucional relacionado con el resguardo de la integridad pública y el impacto que tiene la Transparencia para el perfeccionamiento Institucional y como el cambio regulatorio conlleva beneficios institucionales, esto con la finalidad de combatir la corrupción en la administración pública, en los casos de financiamiento irregular de la política o a la apropiación indebida de los recursos públicos.</p><p> </p>
Correlation Between Experiences of Artistic Creative Self-Expression and Life Experiences in Crisis Conditions
Authors: Kalēja-Gasparoviča Daiga 
Published: August 2018

ABSTRACT
Contemporary conditions determine a relationship between the quality of individual’s life andindividually developed creative abilities: the ability to adapt to extraordinary situations andcircumstances of life, flexibility in thought and action. The studies of visual arts provide anopportunity of enriching one’s experience in creative activities, at the same time facilitating thedevelopment of creative abilities. Experiences acquired earlier in life (impressions, low selfesteemand negative experiences) affect artistic creative self-expression and enhanced creativeexperiences, accordingly, affect the quality of life.

The aim of the article is to reveal and justify the correlations between the personal experiences of
artistic creative self-expression and personal life experiences. Methods used in this study: review
of scientific literature and empirical methods: observation and interviews.

Individual’s creative personal experiences, acquired through artistic creative work in visual
arts have a direct link with the quality of life and its improvement. While studying individual’s
opportunities for creative development acquiring the study content of visual arts education
through studies and the opportunities for improving the quality of life, strong correlative
links between experience, quality of life, creative resources and self-expression have been
established.
Exergy Analysis of a Domestic Refrigerator
Authors: Mahdi Louay Abd Al-Azez , Mohammad Wahid S. , Mahmood Samir Akram 
Published: August 2018

An energy and exergy thermodynamic analysis using EES program was done for a domestic refrigerator working with R-134a using vapor compression refrigeration cycle. The analysis deals with the system component, i.e. compressor, condenser, evaporator and the expansion device. The analysis depends on the entropy generation minimization approach to improve the refrigerator performance by exploring the optimum design points. These design points were derived from three different theories governing the entropy generation minimization using exergy analyzing method. These theories were first applied to find the optimum balance between the hot inner condenser area and the cold inner evaporator area of the refrigerator and between its hot and cold thermal conductances. Nine types of condensers were used according to its internal surface area and thermal conductance, in order to reach the minimum entropy generation in the refrigerator. The results showed that the compressor has the lowest exergy efficiency of 25%. The expansion device was the second component after the compressor with exergy efficiency of 92%, followed by the condenser with an efficiency of 93%. The evaporator was found to have an exergy efficiency of 98 %. The experimental tests were repeated for the nine condensers sizes with three different ambient temperatures 25℃, 30℃ and 35℃. The exergy analysis showed that the design of the refrigerator mainly depends on thermal conductance calculations rather than the surface inner area estimation.
Synthesis, properties and EDM behavior of 10 wt.-% ZrB2 reinforced AA7178 matrix composites
Authors: Kumar Sundaram Dinesh , Ravichandran Manickam 
Published: August 2018

Abstract
The present study outlines the optimization of process parameters in the EDM of AA7178-10 wt.-% ZrB2 composites. The composites were fabricated by using stir casting and the mechanical properties are evaluated. The mechanical properties of AA7075, AA7178 and AA7178-10 wt.-% ZrB2 composites were reported. Scanning electron microscope (SEM) and energy dispersive spectrometry (EDS) analysis were used to characterize the composites. The fabricated composite material was machined using different process parameters based on Taguchi's L9 orthogonal array. Parameters such as current (I), pulse on time (PT-on) and pulse off time (PT-off) were varied. The response variables measured for the analysis are material removal rate (MRR) and surface roughness (SR). From the SN Ratio (SNR) analysis, it was observed that, current is the significant factor affecting both MRR and SR. ANOVA analysis was carried out to determine the percentage contribution of each factor to the responses. Further, a verification experiment was performed to confirm the performance of optimum parameters.
Hipertensão arterial na infância: um estudo de revisão
Authors: Dias da Silva Andressa , De Oliveira Jaqueline Angelica , Immich Isabel Cristina , De Pellegrin Kratz Cristiane 
Published: August 2018

<span>O número de casos de hipertensão arterial sistêmica (HAS) cresce anualmente. Estima-se que 36 milhões de indivíduos adultos apresentem esta patologia, acarretando alto custo socioeconômico. Os fatores de risco incluem dislipidemia, obesidade abdominal, intolerância à glicose e diabetes mellitus. Este estudo objetivou trazer uma abordagem multidisciplinar dos fatores que contribuem para o comprometimento dos níveis normais de pressão arterial (PA) em crianças e adolescentes, além de investigar os possíveis tratamentos farmacológicos e não farmacológicos desta enfermidade. A HAS está relacionada ao aumento do número de indivíduos com sobrepeso, excesso de sódio nos alimentos, consumo precoce de álcool e com o sedentarismo. Há indícios de que a progressão desta seja consequência dos comportamentos e hábitos na infância e adolescência, que implicam na relação da hipertensão na infância com a idade adulta. Crianças com elevações de PA têm predisposição a tornarem-se adultos hipertensos, ainda, as alterações leves da pressão arterial em idades precoces se traduzem em hipertensão com lesão orgânica no adulto, podendo resultar em danos na retina, rins, coração, entre outras complicações. Desta forma, é de grande importância o manejo correto tanto do diagnostico quanto da terapêutica da hipertensão na infância, ressaltando a importância da atenção primária à saúde da criança. </span>
ADHESIVE COMPOUND FOR PRODUCTION OF WOOD CHIPBOARD COMPOSITE MATERIALS
Authors: Pikulev V. S. , Sarkisov Yu. S. , Gorlenko N. P. , Klopotov A. A. , Rahmanova I. A. 
Published: August 2018

Currently, the chipboard production is a priority direction in the development of woodworking industry. In addition to purely technological aspects, the environmental safety of chipboard production is the most relevant, which is reflected in the modern patent, scientific and technical literature. One of the main ways to improve the environmental safety and efficiency of the chipboard production is a directed modification of urea-formaldehyde resin, the main binder, in order to significantly change the emission of free formaldehyde from finished structures. This problem is solved by modifying both the binder and the hardener. Ammonium chloride, oxalic acid, hydrochloric acid, ammonium silicofluoride, combined hardener in the composition of ammonium chloride and ammonia water and others are used as a hardener, and a polyacrylamide solution is used as resin modifier. The gas phase of wood chipboards aged at 1100 °C for 30 min was studied using a method of the vapor-phase gas chromatographic analysis with the mass spectrometer detection. Results show that polyacrylamide sample with modifying additives has the smallest quantity of components releasing in the gas phase. Concerning gas emission, all studied wood chipboard samples meet the sanitary rules for the use of polymeric materials in construction and furniture production and the sanitary and hygienic assessment of polymer and polymer-containing building materials and structures intended for use in the construction of residential, public and industrial buildings.
WEIRD: Wide-orbit Exoplanet Search with InfraRed Direct Imaging
Authors: Baron Frédérique , Artigau Étienne , Rameau Julien , Lafrenière David , Gagné Jonathan , Malo Lison , Albert Loïc , Naud Marie-Eve , Doyon René , Janson Markus , Delorme Philippe , Beichman Charles 
Published: August 2018

Abstract
We report results from the Wide-orbit Exoplanet search with InfraRed Direct imaging, or WEIRD, a survey designed to search for Jupiter-like companions on very wide orbits (1000–5000 au) around young stars (<120 Myr) that are known members of moving groups in the solar neighborhood (<70 pc). Companions that share the same age, distance, and metallicity as their host while being on large enough orbits to be studied as “isolated” objects make prime targets for spectroscopic observations, and they are valuable benchmark objects for exoplanet atmosphere models. The search strategy is based on deep imaging in multiple bands across the near-infrared domain. For all 177 objects of our sample,

, J, [3.6], and [4.5] images were obtained with CFHT/MegaCam, GEMINI/GMOS, CFHT/WIRCam, GEMINI/Flamingos-2, and Spitzer/IRAC. Using this set of four images per target, we searched for sources with red

and [3.6]–[4.5] colors, typically reaching good completeness down to 2

companions, while going down to 1

for some targets, at separations of 1000–5000 au. The search yielded four candidate companions with the expected colors, but they were all rejected through follow-up proper motion observations. Our results constrain the occurrence of 1–13

planetary-mass companions on orbits with a semimajor axis between 1000 and 5000 au at less than 0.03, with a 95% confidence level.
MOA-2015-BLG-337: A Planetary System with a Low-mass Brown Dwarf/Planetary Boundary Host, or a Brown Dwarf Binary
Authors: Miyazaki S. , Sumi T. , Bennett D. P. , Gould A. , Udalski A. , Bond I. A. , Koshimoto N. , Nagakane M. , Rattenbury N. , Abe F. , Bhattacharya A. , Barry R. , Donachie M. , Fukui A. , Hirao Y. , Itow Y. , Kawasaki K. , Li M. C. A. , Ling C. H. , Matsubara Y. , Matsuo T. , Muraki Y. , Ohnishi K. , Ranc C. , Saito T. , Sharan A. , Shibai H. , Suematsu H. , Suzuki D. , Sullivan D. J. , Tristram P. J. , Yamada T. , Yonehara A. ,   (MOA collaboration), KozŁowski S. , Mróz P. , Pawlak M. , Poleski R. , Pietrukowicz P. , Skowron J. , Soszyński I. , Szymański M. K. , Ulaczyk K. ,   (OGLE collaboration), Albrow M. D. , Chung S.-J. , Han C. , Jung Y. K. , Hwang K.-H. , Ryu Y.-H. , Shin I.-G. , Shvartzvald Y. , Yee J. C. , Zang W. , Zhu W. , Cha S.-M. , Kim D.-J. , Kim H.-W. , Kim S.-L. , Lee C.-U. , Lee D.-J. , Lee Y. , Park B.-G. , Pogge R. W. ,   (KMTNet collaboration)
Published: August 2018

Abstract
We report on the discovery and analysis of the short-timescale binary-lens microlensing event, MOA-2015-BLG-337. The lens system could be a planetary system with a very low-mass host, around the brown dwarf (BD)/planetary-mass boundary, or a BD binary. We found two competing models that explain the observed light curves with companion/host mass ratios of q ∼ 0.01 and ∼0.17, respectively. A significant finite source effect in the best-fit planetary model (q ∼ 0.01) reveals a small angular Einstein radius of θ
E ≃ 0.03 mas, which favors a low-mass lens. We obtain the posterior probability distribution of the lens properties from a Bayesian analysis. The results for the planetary models strongly depend on a power-law index in planetary-mass regime, α
pl, in the assumed mass function. In summary, there are two solutions of the lens system: (1) a BD/planetary-mass boundary object orbited by a super-Neptune (the planetary model with α
pl = 0.49) and (2) a BD binary (the binary model). If the planetary models are correct, this system can be one of a new class of planetary system, having a low host mass and also a planetary-mass ratio (q < 0.03) between the companion and its host. The discovery of the event is important for the study of planetary formation in very low-mass objects. In addition, it is important to consider all viable solutions in these kinds of ambiguous events in order for the future comprehensive statistical analyses of planetary/binary microlensing events.
Secular Evolution Driven by Massive Eccentric Disks/Rings: An Apsidally Aligned Case
Authors: Davydenkova Irina , Rafikov Roman R. 
Published: August 2018

Abstract
Massive eccentric disks (gaseous or particulate) orbiting a dominant central mass appear in many astrophysical systems, including planetary rings, protoplanetary and accretion disks in binaries, and nuclear stellar disks around supermassive black holes in galactic centers. We present an analytical framework for treating the nearly Keplerian secular dynamics of test particles driven by the gravity of an eccentric, apsidally aligned, zero-thickness disk with arbitrary surface density and eccentricity profiles. We derive a disturbing function describing the secular evolution of coplanar objects, which is explicitly related (via one-dimensional, convergent integrals) to the disk surface density and eccentricity profiles without using any ad hoc softening of the potential. Our analytical framework is verified via direct orbit integrations, which show it to be accurate in the low-eccentricity limit for a variety of disk models (for disk eccentricity ≲0.1–0.2). We find that free precession in the potential of a disk with a smooth surface density distribution can naturally change from prograde to retrograde within the disk. Sharp disk features—edges and gaps—are the locations where this tendency is naturally enhanced, while the precession becomes very fast. Radii where free precession changes sign are the locations where substantial (formally singular) growth of the forced eccentricity of the orbiting objects occurs. Based on our results, we formulate a self-consistent analytical framework for computing an eccentricity profile for an aligned, eccentric disk (with a prescribed surface density profile) capable of precessing as a solid body under its own self-gravity.
The Proper Motion Field of the Small Magellanic Cloud: Kinematic Evidence for Its Tidal Disruption
Authors: Zivick Paul , Kallivayalil Nitya , van der Marel Roeland P. , Besla Gurtina , Linden Sean T. , Kozłowski Szymon , Fritz Tobias K. , Kochanek C. S. , Anderson J. , Sohn Sangmo Tony , Geha Marla C. , Alcock Charles R. 
Published: August 2018

Abstract
We present a new measurement of the systemic proper motion of the Small Magellanic Cloud (SMC), based on an expanded set of 30 fields containing background quasars and spanning a ∼3 year baseline, using the Hubble Space Telescope (HST) Wide Field Camera 3. Combining this data with our previous five HST fields, and an additional eight measurements from the Gaia-Tycho Astrometric Solution Catalog, brings us to a total of 43 SMC fields. We measure a systemic motion of μ

W
= −0.82 ± 0.02 (random) ± 0.10 (systematic) mas yr−1 and μ

N
= −1.21 ± 0.01 (random) ± 0.03 (systematic) mas yr−1. After subtraction of the systemic motion, we find little evidence for rotation, but find an ordered mean motion radially away from the SMC in the outer regions of the galaxy, indicating that the SMC is in the process of tidal disruption. We model the past interactions of the Clouds with each other based on the measured present-day relative velocity between them of 103 ± 26 km s−1. We find that in 97% of our considered cases, the Clouds experienced a direct collision 147 ± 33 Myr ago, with a mean impact parameter of 7.5 ± 2.5 kpc.
Filamentary Structures and Star Formation Activity in the Sites S234, V582, and IRAS 05231+3512
Authors: Dewangan L. K. , Baug T. , Ojha D. K. , Zinchenko I. , Luna A. 
Published: August 2018

Abstract
To investigate ongoing physical processes, we present the results of observations of the sites S234, V582, and IRAS 05231+3512 situated toward l = 171.°7–174.°1. Based on the CO line data, we find that these sites are not physically connected, and contain at least one filament (with length >7 pc). The observed line masses (M
line,obs) of the filaments associated with V582 and IRAS 05231+3512 are ∼37 and ∼28 M
⊙ pc−1, respectively. These filaments are characterized as thermally supercritical, and harbor several clumps. Groups of infrared-excess sources and massive B-type stars are observed toward the filament containing V582, while very little star formation (SF) activity is found around IRAS 05231+3512. Our results favor a radial collapse scenario in the filaments harboring V582 and IRAS 05231+3512. In the site S234, two filaments (i.e., ns1 (M
line,obs ∼ 130 M
⊙ pc−1) and ns2 (M
line,obs ∼ 45 M
⊙ pc−1)) are identified as thermally supercritical. An extended temperature structure at 27–30 K surrounds the relatively cold (∼19 K) ∼8.9 pc long filament ns1. At least four condensations (M
clump ∼ 70–300 M
⊙) are seen in ns1, and are devoid of 610 MHz radio emission as observed by the Giant Metrewave Radio Telescope. The filament ns2 hosting clumps is devoid of ongoing SF, and could be at an early stage of fragmentation. Intense SF activity, with an SF efficiency ∼3.3% and SF rate ∼40–20 M
⊙ Myr−1 (for t
sf ∼ 1–2 Myr), is observed in ns1. The feedback of massive stars in S234 seems to explain the observed SF in the filament ns1.
Ring Galaxies Through Off-center Minor Collisions by Tuning Bulge-to-disk Mass Ratio of Progenitors
Authors: Chen Guangwen , Wu Xufen , Kong Xu , Liu Wen-Juan , Zhao HongSheng 
Published: August 2018

Abstract
Collisional ring galaxies (CRGs) are formed through off-center collisions between a target galaxy and an intruder dwarf galaxy. We study the mass distribution and kinematics of CRGs by tuning the bulge-to-disk mass ratio (B/D) for the progenitor; i.e., the target galaxy. We find that the lifetime of the ring correlates with the initial impact velocity vertical to the disk plane (i.e., v

z0). Three orbits for the collisional galaxy pair, on which clear and asymmetric rings form after collisions, are selected to perform the N-body simulations at different values of B/D for the progenitor. It is found that the ring structures are the strongest for CRGs with small values of B/D. The Sérsic index, n, of the central remnant in the target galaxy becomes larger after collision. Moreover, the Sérsic index of a central remnant strongly correlates with the initial value of B/D for the progenitor. A bulge-less progenitor results in a late-type object in the center of the ring galaxy, whereas a bulge-dominated progenitor leads to an early-type central remnant. Progenitors with B/D ∈ [0.1, 0.3] (i.e., minor bulges) leave central remnants with n ≈ 4. These results provide a possible explanation for the formation of a recently observed CRG with an early-type central nucleus, SDSS J1634+2049. In addition, we find that the radial and azimuthal velocity profiles for a ring galaxy are more sensitive to the B/D than the initial relative velocity of the progenitor.