Inteligencia emocional y empatía: su influencia en la competencia social en Educación Secundaria Obligatoria

La finalidad del presente trabajo es analizar las relaciones existentes entre la competencia social y la inteligencia emocional en estudiantes de Educación Secundaria Obligatoria. Así mismo, también nos proponemos analizar el papel de la empatía y sus relaciones con la competencia social y la inteligencia emocional, ya que en la mayoría de los estudios existentes aparece relacionada de un modo u otro con estos constructos. Los participantes en nuestro estudio fueron 110 estudiantes de primer ciclo de ESO. Los instrumentos empleados fueron: el test EQ-i:YV de BarOn (1997), el Cuestionario Matson de habilidades sociales para adolescentes (Matson, Rotatori, y Helsel, 1983) y el Interpersonal Reactivity Index, IRI (Davis, 1983). Las técnicas de análisis de datos incluyen: análisis de correlación, análisis de regresión múltiple paso a paso y análisis de regresión múltiple de tipo jerárquico. Los resultados obtenidos nos permiten identificar un conjunto de variables que están directamente implicadas en la Competencia social.

Astrophysical parameters of LS 2883 and implications for the PSR B1259-63 gamma-ray binary

Only a few binary systems with compact objects display TeV emission. The physical properties of the companion stars represent basic input for understanding the physical mechanisms behind the particle acceleration, emission, and absorption processes in these so-called gamma-ray binaries. Here we present high-resolution and high signal-to-noise optical spectra of LS 2883, the Be star forming a gamma-ray binary with the young non-accreting pulsar PSR B1259-63, showing it to rotate faster and be significantly earlier and more luminous than previously thought. Analysis of the interstellar lines suggests that the system is located at the same distance as (and thus is likely a member of) Cen OB1. Taking the distance to the association, d = 2.3 kpc, and a color excess of E(B – V) = 0.85 for LS 2883 results in MV ≈ –4.4. Because of fast rotation, LS 2883 is oblate (R eq sime 9.7 R ☉ and R pole sime 8.1 R ☉) and presents a temperature gradient (T eq≈ 27,500 K, log g eq = 3.7; T pole≈ 34,000 K, log g pole = 4.1). If the star did not rotate, it would have parameters corresponding to a late O-type star. We estimate its luminosity at log(L */L ☉) sime 4.79 and its mass at M * ≈ 30 M ☉. The mass function then implies an inclination of the binary system i orb ≈ 23°, slightly smaller than previous estimates. We discuss the implications of these new astrophysical parameters of LS 2883 for the production of high-energy and very high-energy gamma rays in the PSR B1259-63/LS 2883 gamma-ray binary system. In particular, the stellar properties are very important for prediction of the line-like bulk Comptonization component from the unshocked ultrarelativistic pulsar wind.

Assessment of CO2 adsorption capacity on activated carbons by a combination of batch and dynamic tests

In this work, batch and dynamic adsorption tests are coupled for an accurate evaluation of CO2 adsorption performance for three different activated carbons obtained from olives stones by chemical activation followed by physical activation with CO2 at varying times, i.e. 20, 40 and 60 h. Kinetic and thermodynamic CO2 adsorption tests from simulated flue-gas at different temperature and CO2 pressure are carried out both in batch (a manometric equipment operating with pure CO2) and dynamic (a lab-scale fixed-bed column operating with CO2/N2 mixture) conditions. The textural characterization of the activated carbon samples shows a direct dependence of both micropore and ultramicropore volume on the activation time, hence AC60 has the higher contribution. The adsorption tests conducted at 273 and 293 K showed that, when CO2 pressure is lower than 0.3 bar, the lower the activation time the higher CO2 adsorption capacity and a ranking ωeq(AC20)>ωeq(AC40)>ωeq(AC60) can be exactly defined when T= 293 K. This result can be likely ascribed to a narrower pore size distribution of the AC20 sample, whose smaller pores are more effective for CO2 capture at higher temperature and lower CO2 pressure, the latter representing operating conditions of major interest for decarbonation of a flue-gas effluent. Moreover, the experimental results obtained from dynamic tests confirm the results derived from the batch tests in terms of CO2 adsorption capacity. It is important to highlight that the adsorption of N2 on the synthesized AC samples can be considered negligible. Finally, the importance of a proper analysis of characterization data and adsorption experimental results is highlighted for a correct assessment of CO2 removal performances of activated carbons at different CO2 pressure and operating temperature.

Estudio de la inteligencia emocional en alumnos de enseñanza secundaria: influencia del sexo y del nivel educativo de los estudiantes y su relación con el rendimiento académico

Los objetivos de este estudio fueron analizar la inteligencia emocional entre alumnos de secundaria y la influencia del sexo, nivel educativo y rendimiento académico. La muestra fue de 151 alumnos. Se utilizó el EQ-i: YV y el promedio de calificaciones. Los resultados indicaron una fuerte relación entre inteligencia emocional y rendimiento académico, y diferencias significativas en función del sexo y nivel educativo.