Hot thermal X-ray emission from the Be star HD 119682

We present an analysis of a series of four consecutive Chandra high-resolution transmission gratings observations, amounting to a total of 150 ks, of the Be X-ray source HD 119682 (=1WGA J1346.5–6255), a member of the new class of γ Cas analogs. The Chandra light curve shows significant brightness variations on timescales of hours. However, the spectral distribution appears rather stable within each observation and during the whole campaign. A detailed analysis is not able to detect any coherent pulsation up to a frequency of 0.05 Hz. The Chandra High Energy Transmission Gratings spectrum seems to be devoid of any strong emission line, including Fe Kα fluorescence. The continuum is well described with the addition of two collisionally ionized plasmas of temperatures kT ≈ 15 keV and 0.2 keV, respectively, by the apec model. Models using photoionized plasma components (mekal) or non-thermal components (powerlaw) give poorer fits, providing support for the pure thermal scenario. These two components are absorbed by a single column with N H = (0.20+0.15 –0.03) × 1022 cm–2 compatible with the interstellar value. We conclude that HD 119682 can be regarded as a pole-on γ Cas analog.

Evaluación de la calidad de vida relacionada con la salud mediante las láminas Coop-Wonca en una población de hemodiálisis

Ante la necesidad de disponer de instrumentos que permitan medir calidad de vida relacionada con la salud (CVRS) de una manera ágil y rápida, nos planteamos estudiar, en un grupo de pacientes en hemodiálisis, las propiedades de medición de las láminas Coop-Wonca con el objetivo de establecer si reúnen las condiciones para su uso rutinario en este tipo de pacientes. Métodos: Estudio transversal en 163 pacientes de hemodiálisis (106 varones y 57 mujeres) procedentes de 3 centros. Para medir la CVRS de la población estudiada se ha utilizado la versión validada española de las láminas Coop-Wonca completa. Este cuestionario comprende nueve dimensiones de función y bienestar de un único ítem: 1.– Forma física; 2.–Sentimientos; 3.–Actividades cotidianas; 4.–Actividades sociales; 5.–Cambio en el estado de salud; 6.–Estado de salud; 7.–Dolor; 8.–Apoyo social; y 9.–Calidad de vida en general. Las posibles respuestas se puntúan de 1 a 5, siendo las puntuaciones mayores las que reflejan una peor salud percibida. El instrumento permite la obtención de un índice (Coop total) que es un sumatorio de las puntuaciones de todas las dimensiones salvo la 5 (Cambio en el estado de salud). Resultados: El tiempo medio de cumplimentación del cuestionario fue inferior a 5 minutos. Las láminas resultaron fácilmente comprensibles para los pacientes y la autoadministración de las mismas no planteó problemas. Las puntuaciones más altas (peor CVRS) se obtuvieron en las dimensiones «forma física» (3,66 ± 0,8) y «estado de salud» (3,43 ± 0,8), y la menor (mejor CVRS) en la dimensión «actividades sociales» (1,98 ± 1,3). Entre los principales factores asociados a un peor estado de salud percibida figuran el sexo (mujer), la comorbilidad (presencia de diabetes y/o hepatopatía), la situación laboral (pensionista) y el medio de transporte (taxi-ambulancia). Un mayor tiempo en hemodiálisis se asoció a peores puntuaciones en las dimensiones «calidad de vida en general» y «Dolor». Los pacientes que se trasladaban en taxi o ambulancia presentaban peores puntuaciones en las dimensiones «Forma física», «Actividades cotidianas» y «Estado de salud». Una mayor se asoció a peor puntuación en «Forma física». Un número elevado de fármacos prescritos (más de seis) se asoció a peor puntuación en las dimensiones «Forma física», «Actividades sociales» y «Apoyo social». Los varones, los viudos y los solteros puntuaron peor en «Apoyo social». Los pacientes con mayor nivel de estudios mostraron puntuaciones más altas (peor CVRS) en la dimensión «Forma física». Conclusiones: Las láminas Coop-Wonca podrían ser un buen instrumento de medida de CVRS en los pacientes de hemodiálisis, por la rapidez de su cumplimentación y por ser de fácil comprensión lo que favorece la autoadministración que evita el posible sesgo del entrevistador. Todo ello favorecería su uso rutinario como indicador par valorar la evolución en el tiempo de la CVRS de los pacientes en hemodiálisis. No obstante, se precisan estudios ulteriores que permitan evaluar en mayor profundidad las propiedades psicométricas del instrumento en este tipo de pacientes.

Evaluación del bienestar espiritual en pacientes en hemodiálisis

Introducción: Se define la espiritualidad como la búsqueda personal de propósito y significado en la vida, pudiendo incorporar o no la religión. En este artículo se presenta el desarrollo y la aplicación de una medida de bienestar espiritual a una muestra de pacientes en hemodiálisis. Material y métodos: El instrumento básico empleado se denomina Cuestionario del Sentido de la Vida (Meaning in Life Scale, MiLS), con 21 ítems y cuatro escalas: Propósito, Falta de significado, Paz y Beneficios de la espiritualidad. También se proporciona una puntuación global de espiritualidad. Además, se registraron variables de tipo clínico (tiempo en hemodiálisis, índice de comorbilidad de Charlson) y sociodemográfico (edad, género), así como estimaciones del estado de salud, calidad de vida (general y actual), felicidad personal, el grado de religiosidad y la creencia en la existencia de vida ultraterrena. Se ha utilizado un diseño transversal con 94 pacientes en hemodiálisis. Resultados: Los resultados muestran que la versión española de este instrumento (MiLS-Sp) es una medida de bienestar espiritual con garantías psicométricas de calidad (fiabilidad, validez), adecuada para evaluar las complejas exigencias generadas por la problemática de salud del paciente en hemodiálisis. El bienestar espiritual se relaciona significativamente con diversas variables de calidad de vida, percepción de salud, felicidad personal o religiosidad. No existe una relación significativa entre las puntuaciones de espiritualidad y la edad, el sexo, el tiempo en diálisis o el índice de comorbilidad. El grado de bienestar espiritual de estos pacientes es relativamente bajo. Conclusión: La espiritualidad parece desempeñar un papel importante en el bienestar psicológico, el estado de salud y la calidad de vida percibidos por el paciente en hemodiálisis. El grado de bienestar espiritual de estos pacientes es relativamente bajo. Estos resultados sugieren que considerar y evaluar el grado de bienestar espiritual en los pacientes en hemodiálisis puede ser de utilidad para la práctica clínica.

Transacciones en SQL Server

Una introducción a los objetivos y contenidos de la sesión 2 del curso de Bases de Datos dentro del Máster Universitario en Desarrollo de Aplicaciones y Servicios Web de la Universidad de Alicante. Se describe someramente qué se entiende por una transacción y se nombran los niveles de aislamiento en SQL Server. Todo enfocado a la realización de los ejercicios-demostraciones de esos niveles de aislamiento. Ingenuo y con fallos de encuadre e iluminación clamorosos, pero no tiene más ambiciones que la de dejar constancia de algunas de las cosas que se dijeron en clase.

Paginación en SQL Server

Una introducción a los objetivos y contenidos de la sesión 3 del curso de Bases de Datos dentro del Máster Universitario en Desarrollo de Aplicaciones y Servicios Web de la Universidad de Alicante. El trabajo que permite la calificación de esta primera parte del curso se basa, precisamente, en lo que se describe en este vídeo. La paginación de resultados es una técnica que pretende agilizar el manejo remoto de grandes cantidades de datos. El ejemplo clásico es la navegación por un catálogo de productos. Si es el servidor el que, por el procedimiento que sea, divide la lista completa en páginas y solo envía una de ellas al cliente, estamos ahorrando en tiempo y uso de red. En SQL Server, para esta tarea, es fácil encontrar opiniones que desaconsejan el uso de cursores puesto que se supone que el entorno objetivo es de alta concurrencia. No obstante, se puede usar TOP() y ROW_NUMBER(). La sesión consiste en una serie de ejemplos sobre todas estas herramientas.

On the nature of the galactic early-B hypergiants

Aims. Despite their importance to a number of astrophysical fields, the lifecycles of very massive stars are still poorly defined. In order to address this shortcoming, we present a detailed quantitative study of the physical properties of four early-B hypergiants (BHGs) of spectral type B1-4 Ia+; Cyg OB2 #12, ζ1 Sco, HD 190603 and BP Cru. These are combined with an analysis of their long-term spectroscopic and photometric behaviour in order to determine their evolutionary status. Methods. Quantitative analysis of UV–radio photometric and spectroscopic datasets was undertaken with a non-LTE model atmosphere code in order to derive physical parameters for comparison with apparently closely related objects, such as B supergiants (BSGs) and luminous blue variables (LBVs), and theoretical evolutionary predictions. Results. The long-term photospheric and spectroscopic datasets compiled for the early-B HGs revealed that they are remarkably stable over long periods ( ≥ 40 yrs), with the possible exception of ζ1 Sco prior to the 20th century; in contrast to the typical excursions that characterise LBVs. Quantitative analysis of ζ1 Sco, HD 190603 and BP Cru yielded physical properties intermediate between BSGs and LBVs; we therefore suggest that BHGs are the immediate descendants and progenitors (respectively) of such stars, for initial masses in the range ~30−60 M⊙. Comparison of the properties of ζ1 Sco with the stellar population of its host cluster/association NGC 6231/Sco OB1 provides further support for such an evolutionary scenario. In contrast, while the wind properties of Cyg OB2 #12 are consistent with this hypothesis, the combination of extreme luminosity and spectroscopic mass (~110 M⊙) and comparatively low temperature means it cannot be accommodated in such a scheme. Likewise, despite its co-location with several LBVs above the Humphreys-Davidson (HD) limit, the lack of long term variability and its unevolved chemistry apparently excludes such an identification. Since such massive stars are not expected to evolve to such cool temperatures, instead traversing an O4-6Ia → O4-6Ia+ → WN7-9ha pathway, the properties of Cyg OB2 #12 are therefore difficult to understand under current evolutionary paradigms. Finally, we note that as with AG Car in its cool phase, despite exceeding the HD limit, the properties of Cyg OB2 #12 imply that it lies below the Eddington limit – thus we conclude that the HD limit does not define a region of the HR diagram inherently inimical to the presence of massive stars.

A Be-type star with a black-hole companion

Stellar-mass black holes have all been discovered through X-ray emission, which arises from the accretion of gas from their binary companions (this gas is either stripped from low-mass stars or supplied as winds from massive ones). Binary evolution models also predict the existence of black holes accreting from the equatorial envelope of rapidly spinning Be-type stars1, 2, 3 (stars of the Be type are hot blue irregular variables showing characteristic spectral emission lines of hydrogen). Of the approximately 80 Be X-ray binaries known in the Galaxy, however, only pulsating neutron stars have been found as companions2, 3, 4. A black hole was formally allowed as a solution for the companion to the Be star MWC 656 (ref. 5; also known as HD 215227), although that conclusion was based on a single radial velocity curve of the Be star, a mistaken spectral classification6 and rough estimates of the inclination angle. Here we report observations of an accretion disk line mirroring the orbit of MWC 656. This, together with an improved radial velocity curve of the Be star through fitting sharp Fe ii profiles from the equatorial disk, and a refined Be classification (to that of a B1.5–B2 III star), indicates that a black hole of 3.8 to 6.9 solar masses orbits MWC 656, the candidate counterpart of the γ-ray source AGL J2241+4454 (refs 5, 6). The black hole is X-ray quiescent and fed by a radiatively inefficient accretion flow giving a luminosity less than 1.6 × 10−7 times the Eddington luminosity. This implies that Be binaries with black-hole companions are difficult to detect in conventional X-ray surveys.

Astrophysical parameters of the peculiar X-ray transient IGR J11215−5952

Context. The current generation of X-ray satellites has discovered many new X-ray sources that are difficult to classify within the well-described subclasses. The hard X-ray source IGR J11215−5952 is a peculiar transient, displaying very short X-ray outbursts every 165 days. Aims. To characterise the source, we obtained high-resolution spectra of the optical counterpart, HD 306414, at different epochs, spanning a total of three months, before and around the 2007 February outburst with the combined aims of deriving its astrophysical parameters and searching for orbital modulation. Methods. We fit model atmospheres generated with the fastwind code to the spectrum, and used the interstellar lines in the spectrum to estimate its distance. We also cross-correlated each individual spectrum to the best-fit model to derive radial velocities. Results. From its spectral features, we classify HD 306414 as B0.5 Ia. From the model fit, we find Teff ≈ 24 700 K and log g ≈ 2.7, in good agreement with the morphological classification. Using the interstellar lines in its spectrum, we estimate a distance to HD 306414 d ≳ 7 kpc. Assuming this distance, we derive R∗ ≈ 40 R⊙ and Mspect ≈ 30 M⊙ (consistent, within errors, with Mevol ≈ 38 M⊙, and in good agreement with calibrations for the spectral type). Analysis of the radial velocity curve reveals that radial velocity changes are not dominated by the orbital motion, and provide an upper limit on the semi-amplitude for the optical component Kopt ≲ 11 ± 6 km   s-1. Large variations in the depth and shape of photospheric lines suggest the presence of strong pulsations, which may be the main cause of the radial velocity changes. Very significant variations, uncorrelated with those of the photospheric lines are seen in the shape and position of the Hα emission feature around the time of the X-ray outburst, but large excursions are also observed at other times. Conclusions. HD 306414 is a normal B0.5 Ia supergiant. Its radial velocity curve is dominated by an effect that is different from binary motion, and is most likely stellar pulsations. The data available suggest that the X-ray outbursts are caused by the close passage of the neutron star in a very eccentric orbit, perhaps leading to localised mass outflow.

Clinical and quality of life data correlation with a single-optic accommodating intraocular lens

Purpose: To examine a single-optic accommodating intraocular lens (IOL) visual performance by correlating IOL implanted eyes’ defocus curve with the intraocular aberrometric profile and the impact on the quality of life (QOL). Methods: Prospective consecutive case series study including a total of 25 eyes of 14 patients with ages ranging between 52 and 79 years old. All cases underwent cataract surgery with implantation of the single-optic accommodating IOL Crystalens HD (Bausch & Lomb). Distance and near visual acuity outcomes, intraocular aberrations, the defocus curve and QOL (NEI VFQ-25) were evaluated 3 months after surgery. Results: A significant improvement in distance visual acuity was found postoperatively (p = 0.02). Mean postoperative LogMAR uncorrected near visual acuity was 0.44 ± 0.23 (20/30). 60% of eyes had a postoperative addition between 0 and 1.5 diopters (D). The defocus curve showed an area of maximum visual acuity for the levels of defocus corresponding to distance and intermediate vision (−1 to +0.5 D). Postoperative intermediate visual acuity correlated significantly some QOL indices (r ≥ 0.51, p ≤ 0.03; difficulty in going down steps or seeing how people react to things that patient says) as well as with J0 component of manifest cylinder. Postoperative distance-corrected near visual acuity correlated significantly with age (r = 0.65, p < 0.01). Conclusions: This accommodating IOL seems to be able to restore the distance visual function as well as to provide an improvement in intermediate and near vision with a significant impact on patient's QOL, although limited by age and astigmatism. Future studies with larger sample sizes should confirm all these trends.

Corneal Biomechanics, Retinal Nerve Fiber Layer, and Optic Disc in Children

Purpose: To evaluate the possible associations between corneal biomechanical parameters, optic disc morphology, and retinal nerve fiber layer (RNFL) thickness in healthy white Spanish children. Methods: This cross-sectional study included 100 myopic children and 99 emmetropic children as a control group, ranging in age from 6 to 17 years. The Ocular Response Analyzer was used to measure corneal hysteresis (CH) and corneal resistance factor. The optic disc morphology and RNFL thickness were assessed using posterior segment optical coherence tomography (Cirrus HD-OCT). The axial length was measured using an IOLMaster, whereas the central corneal thickness was measured by anterior segment optical coherence tomography (Visante OCT). Results: The mean (±SD) age and spherical equivalent were 12.11 (±2.76) years and −3.32 (±2.32) diopters for the myopic group and 11.88 (±2.97) years and +0.34 (±0.41) diopters for the emmetropic group. In a multivariable mixed-model analysis in myopic children, the average RNFL thickness and rim area correlated positively with CH (p = 0.007 and p = 0.001, respectively), whereas the average cup-to-disc area ratio correlated negatively with CH (p = 0.01). We did not observe correlation between RNFL thickness and axial length (p = 0.05). Corneal resistance factor was only positively correlated with the rim area (p = 0.001). The central corneal thickness did not correlate with the optic nerve parameters or with RNFL thickness. These associations were not found in the emmetropic group (p > 0.05 for all). Conclusions: The corneal biomechanics characterized with the Ocular Response Analyzer system are correlated with the optic disc profile and RNFL thickness in myopic children. Low CH values may indicate a reduction in the viscous dampening properties of the cornea and the sclera, especially in myopic children.

Positional accommodative intraocular lens power error induced by the estimation of the corneal power and the effective lens position

Purpose: To evaluate the predictability of the refractive correction achieved with a positional accommodating intraocular lenses (IOL) and to develop a potential optimization of it by minimizing the error associated with the keratometric estimation of the corneal power and by developing a predictive formula for the effective lens position (ELP). Materials and Methods: Clinical data from 25 eyes of 14 patients (age range, 52–77 years) and undergoing cataract surgery with implantation of the accommodating IOL Crystalens HD (Bausch and Lomb) were retrospectively reviewed. In all cases, the calculation of an adjusted IOL power (PIOLadj) based on Gaussian optics considering the residual refractive error was done using a variable keratometric index value (nkadj) for corneal power estimation with and without using an estimation algorithm for ELP obtained by multiple regression analysis (ELPadj). PIOLadj was compared to the real IOL power implanted (PIOLReal, calculated with the SRK-T formula) and also to the values estimated by the Haigis, HofferQ, and Holladay I formulas. Results: No statistically significant differences were found between PIOLReal and PIOLadj when ELPadj was used (P = 0.10), with a range of agreement between calculations of 1.23 D. In contrast, PIOLReal was significantly higher when compared to PIOLadj without using ELPadj and also compared to the values estimated by the other formulas. Conclusions: Predictable refractive outcomes can be obtained with the accommodating IOL Crystalens HD using a variable keratometric index for corneal power estimation and by estimating ELP with an algorithm dependent on anatomical factors and age.