Importancia de la policía especializada en la etapa de indagación patrimonial en el proceso de extinción de dominio

Con el pasar del tiempo los ilícitos penales en nuestro país han aumentado de una manera desmesurada, permitiendo que personas al margen de la Ley incrementen su patrimonio con el dinero obtenido de diversos ilícitos penales, por ello, el presente trabajo de investigación ha sido desarrollado desde la óptica del derecho y de conformidad a lo establecido en el decreto legislativo Nº 1373 que regula el proceso de extinción de dominio en el Perú. Por tanto, la presente investigación tiene como principal objetivo describir la importancia de la policía especializada en la etapa de indagación patrimonial en el proceso de extinción de dominio, basado en un enfoque cualitativo de revisión documental, utilizando libros, revistas jurídicas, entre otros con el fin de recabar información útil y pertinente en relación al tema de estudio

Link between method of delivery and childhood overweight or obesity

This study aimed to determine the relationship between the method of delivery and the incidence of overweight or obesity during childhood. This study was conducted on June 2012 to March 2013 in four selected elementary schools in Iligan City, Philippines wherein 96 overweight to obese children between 5-8 years old were selected as respondents through purposive sampling technique. A descriptive-correlational research design was used. To gather the pertinent data and information, a researcher-made questionnaire was employed. The data gathered were then tabulated and analyzed using frequency and percentage distribution, Chi-square test and Spearman correlation coefficient. It was found out that there is no sufficient evidence to harbor a significant relationship between the method of delivery and the incidence of childhood overweight or obesity among the respondents. Thus, other factors should be explored to relate to overweight or obesity in childhoo

Cesárea Electiva y su Repercusión en la Respiración Neonatal. Hospital II – 2 - Minsa, 2013”

This research "elective Caesarean section and its impact on neonatal Respiratory Hospital II - 2 - MINSA, 2013, is a quantitative, retroprospectivo, Analytical, cross-sectional study; aimed at determining the impact of elective Cesarean on neonatal respiration. The study population consisted Of 242 patients and 242 cesarean vaginal birth. The results were that the population was characterized as mostly the age Group of 15 to 25 years 38.4% (93) with elective cesarean Section and vaginal delivery in the age group of 26-35 years to 41.7% (101). 40.5% (98) of women with elective cesarean have primary-school Education and 38.4% (93) with vaginal delivery have high school Degree, according to marital status 41.7% (101) of women With cesarean collective or vaginal delivery have free union. As For occupation women with elective caesarean are housewives in 55.4% (134) and equal to those of vaginal delivery with 47.9% (116). Regarding The place of origin women with elective cesarean come from urban areas with 142 (59%) as well as those of vaginal delivery with 188 (78%). The frequency of elective cesarean section in pregnant women treated at The Hospital II - 2 MINSA is 31.0% (650) and the main causes or indication For elective caesarean study population was the iterative section with 29.3% (71) followed by maternal infections in 25.6% (62). In conclusion statistically elective cesarean if impacts on the occurrence of Neonatal respiratory distress syndrome in patients treated in the Hospital II - 2 - MINSA, higher relative risk of 1.0.La presente investigación “Cesárea electiva y su repercusión en la Respiración neonatal Hospital II – 2 - MINSA, 2013, es un estudio Cuantitativo, retroprospectivo, analítico, de corte transversal; cuyo objetivo es Determinar la repercusión de la cesárea electiva en la respiración neonatal. La población en estudio estuvo conformado por 242 pacientes de parto por Cesárea electiva y 242 de parto vaginal. Los resultados fueron que la población se caracterizó por ser Mayoritariamente del grupo etareo de 15 a 25 años 38.4% (93) con cesárea Electiva y las de parto vaginal del grupo etareo de 26 a 35 años en 41,7% (101). El 40.5% (98) de las mujeres con cesárea electiva cuentan con grado De instrucción primaria y el 38,4% (93) con parto vaginal tienen grado de Instrucción secundaria, según estado civil 41.7% (101) de las mujeres con Cesárea lectiva o parto vaginal tienen unión libre. En cuanto a ocupación las Mujeres con cesárea electiva son amas de casa en 55.4% (134) e igual las De parto vaginal con 47.9% (116). En relación al lugar de procedencia las Mujeres con cesárea electiva proceden de la zona urbana con 142 (59%) al Igual que las de parto vaginal con 188 (78%). La frecuencia de cesárea electiva en parturientas atendidas en el Hospital II – 2 MINSA es de 31.0% (650) y las principales causas o indicación de Cesárea electiva de la población en estudio fue la cesárea iterativa con un 29.3% (71) seguido de las infecciones maternas en 25.6% (62). En conclusión la cesárea electiva estadísticamente si repercute en la Presencia del síndrome de dificultad respiratoria neonatal, en pacientes Atendidas en el Hospital II – 2 – MINSA, riesgo relativo mayor de 1,0.Tesi

A dry electrophysiology electrode using CNT arrays

We describe the concept of a dry electrode sensor for biopotential measurement applications (ENOBIO) designed to eliminate the noise and inconvenience associated to the use of electrolytic gel. ENOBIO uses nanotechnology to remove gel-related noise, as well as maintaining a good contact impedance to minimise interference noise. The contact surface of the electrode will be covered with an array/forest of carbon nanotubes and will also be tested with an Ag/AgCl coating to provide ionic-electronic transduction. The nanotubes are to penetrate the outer layers of the skin, the Stratum Corneum, improving electrical contact. We discuss requirements, skin properties, nanotube penetration and transduction, noise sources, prototype design logic and biocompatibility. A future paper will report test results.Comment: Submitted to Sensors and Actuators, Proceedings of Eurosensors XIX, Barcelona, Spain, 2005. Figure 2 corrected, references correcte

Confronting 3 Dimensional Time-dependent Jet Simulations with HST Observations

We perform state-of-the-art, 3D, time-dependent simulations of magnetized disk winds, carried out to simulation scales of 60 Astronomical Units, in order to confront optical HST observations of protostellar jets. We ``observe'' the optical forbidden line emission produced by shocks within our simulated jets and compare these with actual observations. Our simulations reproduce the rich structure of time varying jets, including jet rotation far from the source, an inner (up to 400 km/s) and outer (less than 100 km/s) component of the jet, and jet widths of up to 20 Astronomical Units in agreement with observed jets. These simulations when compared with the data are able to constrain disk wind models. In particular, models featuring a disk magnetic field with a modest radial spatial variation across the disk are favored.Comment: Accepted for publication in Ap

UMass Amherst Green Building Guidelines v.2 and LEEDv4

Facilities & Campus Services supports sustainability and energy conservation initiatives by providing in-house resources to campus staff as well as designers, contractors and other consultants working with the University. The UMass Amherst Green Building Guidelines v2 and LEED v4 provide a framework for approaching new construction and major renovation projects at UMass Amherst that are undergoing LEED v4 certification by focusing the conversation on those green building aspects that are most important to the campus. They are intended to be the beginning of a dynamic conversation between designers, environmental consultants and constructors, university stakeholders, and users of new high performance buildings

Recipes for stellar jets: results of combined optical/infrared diagnostics

We examine the conditions of the plasma along a sample of 'classical' Herbig-Haro jets located in the Orion and Vela star forming regions, through combined optical-infrared spectral diagnostics. Our sample includes HH 111, HH 34, HH 83, HH 73, HH 24 C/E, HH 24 J, observed at moderate spatial/spectral resolution. The obtained spectra cover a wide wavelength range from 0.6-2.5 um, including many transitions from regions of different excitation conditions. This allows us to probe the density and temperature stratification which characterises the cooling zones behind the shock fronts along the jet. The derived physical parameters (such as the extinction, the electron density and temperature, the ionisation fraction, and the total density) are used to estimate the depletion onto dust grains of Calcium and Iron with respect to solar abundances. This turns out to be between 70% and 0% for Ca and ~90% for Fe, suggesting that the weak shocks present in the beams are not capable of completely destroying the dust grains. We then derive the mass flux rates (Mdot_jet is on average 5 10^-8 M_solar yr^-1) and the associated linear momentum fluxes. The latter are higher than, or of the same order as, those measured in the coaxial molecular flows, suggesting that the flows are jet driven. Finally, we discuss differences between jets in our sample.Comment: 19 pages, 15 figures, accepted by A&

A combined optical/infrared spectral diagnostic analysis of the HH1 jet

Complete flux-calibrated spectra covering the spectral range from 6000 A to 2.5 um have been obtained along the HH1 jet and analysed in order to explore the potential of a combined optical/near-IR diagnostic applied to jets from young stellar objects. Important physical parameters have been derived along the jet using various diagnostic line ratios. This multi-line analysis shows, in each spatially unresolved knot, the presence of zones at different excitation conditions, as expected from the cooling layers behind a shock front. In particular, a density stratification in the jet is evident from ratios of various lines of different critical density. In particular, [FeII] lines originate in a cooling layer located at larger distances from the shock front than that generating the optical lines, where the compression is higher and the temperature is declining. The derived parameters were used to measure the mass flux along the jet, adopting different procedures, the advantages and limitations of which are discussed. dM/dt is high in the initial part of the flow but decreases by about an order of magnitude further out. Conversely, the mass flux associated with the warm molecular material is low and does not show appreciable variations along the jet. We suggest that part of the mass flux in the external regions is not revealed in optical and IR lines because it is associated with a colder atomic component, which may be traced by the far-IR [O I]63 um line. Finally, we find that the gas-phase abundance of refractory species is lower than the solar value suggesting that a significant fraction of dust grains may still be present in the jet beam.Comment: Accepted on Astronomy & Astrophysic