Carme Serrallonga, el plaer de traduir

Carme Serrallonga (Barcelona, 1909-1997) començà a traduir als anys seixanta, en moments de represa de consciència ideològica i literària. Bona coneixedora de diversos idiomes, especialment l’alemany, l’anglès, el francès i l’italià, girà al català unes vint obres del teatre universal dels grans autors. Serrallonga explicava que havia començat a aprendre alemany per poder conèixer a fons l’obra de Brecht, del qual el 1966 traduí La bona persona de Sezuan, a proposta de Ricard Salvat, i cinc obres més. De l’alemany també portà al català autors com Georg Büchner, Heinrich Böll, Friedrich Dürrenmatt, Peter Handke, György Lukács, Goethe, Mozart o Alfred Döblin. A més de l’alta literatura alemanya, Serrallonga féu petites incursions en la literatura anglesa i nord-americana, la italiana i, fins i tot, la sud-africana. El 1983 l’editorial La Galera li encarregà la traducció d’En Jim Botó i en Lluc el maquinista de Michael Ende. En sis anys traduí més de trenta títols de literatura infantil. Ja jubilada, a vuitanta-quatre anys, es posà a estudiar rus pel plaer de poder llegir Anna Akhmàtova i Txèkhov en la seva llengua originària. Abans de morir, treballava en la traducció d’un llibre de poemes de l’autora russa.

Evaluating the impact of filming on the number of errors committed by nursing students to determine the efficacy of simulated clinical situations

Clinic simulation as a training and knowledge method allows people experiment a real event representation with the aim of acquiring knowledge, abilities and aptitudes. The filming of the staging represents a useful tool to review the decisions taken and the actions they did, with the purpose to highlight the strengths, weaknesses and the areas for improvement. The article describes a study carried out by a group of students in second course of nursing, and it tries to evaluate if there is any influence if somebody is filming you during the clinic simulation, does it make you do more errors or not?

Long-term X-ray variability of the microquasar system LS5039/RX J1826.2-1450

We report on the results of the spectral and timing analysis of a BeppoSAX observation of the microquasar system LS 5039/RX J1826.2-1450. The source was found in a low-flux state with Fx(1-10 keV)= 4.7 x 10^{-12} erg cm^{-2} s^{-1}, which represents almost one order of magnitude lower than a previous RXTE observation 2.5 years before. The 0.1--10 keV spectrum is described by an absorbed power-law continuum with photon-number spectral index Gamma=1.8+-0.2 and hydrogen column density of NH=1.0^{+0.4}_{-0.3} x 10^{22} cm^{-2}. According to the orbital parameters of the system the BeppoSAX observation covers the time of an X-ray eclipse should one occur. However, the 1.6-10 keV light curve does not show evidence for such an event, which allows us to give an upper limit to the inclination of the system. The low X-ray flux detected during this observation is interpreted as a decrease in the mass accretion rate onto the compact object due to a decrease in the mass-loss rate from the primary.

MAGIC TeV Gamma-Ray Observations of Markarian 421 during Multiwavelength Campaigns in 2006

Wide-range spectral coverage of blazar-type active galactic nuclei is of paramount importance for understanding the particle acceleration mechanisms assumed to take place in their jets. The Major Atmospheric Gamma Imaging Cerenkov (MAGIC) telescope participated in three multiwavelength (MWL) campaigns, observing the blazar Markarian (Mkn) 421 during the nights of April 28 and 29, 2006, and June 14, 2006. Aims. We analyzed the corresponding MAGIC very-high energy observations during 9 nights from April 22 to 30, 2006 and on June 14, 2006. We inferred light curves with sub-day resolution and night-by-night energy spectra. Methods. MAGIC detects γ-rays by observing extended air showers in the atmosphere. The obtained air-shower images were analyzed using the standard MAGIC analysis chain. Results. A strong γ-ray signal was detected from Mkn 421 on all observation nights. The flux (E > 250 GeV) varied on night-by-night basis between (0.92±0.11) × 10-10 cm-2 s-1 (0.57 Crab units) and (3.21±0.15) × 10-10 cm-2 s-1 (2.0 Crab units) in April 2006. There is a clear indication for intra-night variability with a doubling time of 36± min on the night of April 29, 2006, establishing once more rapid flux variability for this object. For all individual nights γ-ray spectra could be inferred, with power-law indices ranging from 1.66 to 2.47. We did not find statistically significant correlations between the spectral index and the flux state for individual nights. During the June 2006 campaign, a flux substantially lower than the one measured by the Whipple 10-m telescope four days later was found. Using a log-parabolic power law fit we deduced for some data sets the location of the spectral peak in the very-high energy regime. Our results confirm the indications of rising peak energy with increasing flux, as expected in leptonic acceleration models.

Discovery of a High-Energy Gamma-Ray-Emitting Persistent Microquasar

Microquasars are stellar x-ray binaries that behave as a scaled down version of extragalactic quasars. The star LS 5039 is a new microquasar system with apparent persistent ejection of relativistic plasma at a 3 kiloparsec distance from the sun. It may also be associated with a gamma-ray source discovered by the Energetic Gamma Ray Experiment Telescope (EGRET) on board the COMPTON-Gamma Ray Observatory satellite. Before the discovery of LS 5039, merely a handful of microquasars had been identified in the Galaxy, and none of them was detected in high-energy gamma-rays.

Deep GMRT radio observations and a multi-wavelength study of the region around HESS J1858+020

Context. There are a number of very high energy sources in the Galaxy that remain unidentified. Multi-wavelength and variability studies, and catalogue searches, are powerful tools to identify the physical counterpart, given the uncertainty in the source location and extension. Aims. This work carries out a thorough multi-wavelength study of the unidentified, very high energy source HESS J1858+020 and its environs. Methods. We have performed Giant Metrewave Radio Telescope observations at 610 MHz and 1.4 GHz to obtain a deep, low-frequency radio image of the region surrounding HESS J1858+020. We analysed archival radio, infrared, and X-ray data as well. This observational information, combined with molecular data, catalogue sources, and a nearby Fermi gamma-ray detection of unidentified origin, are combined to explore possible counterparts to the very high energy source. Results. We provide with a deep radio image of a supernova remnant that might be related to the GeV and TeV emission in the region. We confirm the presence of an H ii region next to the supernova remnant and coincident with molecular emission. A potential region of star formation is also identified. We identify several radio and X-ray sources in the surroundings. Some of these sources are known planetary nebulae, whereas others may be non-thermal extended emitters and embedded young stellar objects. Three old, background Galactic pulsars also neighbour HESS J1858+020 along the line of sight. Conclusions. The region surrounding HESS J1858+020 is rich in molecular structures and non-thermal objects that may potentially be linked to this unidentified very high energy source. In particular, a supernova remnant interacting with nearby molecular clouds may be a good candidate, but a star forming region, or a non-thermal radio source of yet unclear nature, may also be behind the gamma-ray source. The neighbouring pulsars, despite being old and distant, cannot be discarded as candidates. Further observational studies are needed, however, to narrow the search for a counterpart to the HESS source.

Optical spectroscopy of microquasar candidates at low Galactic latitudes

We report optical spectroscopic observations of a sample of 6 low-galactic latitude microquasar candidates selected by cross-identification of X-ray and radio point source catalogs for |b|<5 degrees. Two objects resulted to be of clear extragalactic origin, as an obvious cosmologic redshift has been measured from their emission lines. For the rest, none exhibits a clear stellar-like spectrum as would be expected for genuine Galactic microquasars. Their featureless spectra are consistent with being extragalactic in origin although two of them could be also highly reddened stars. The apparent non-confirmation of our candidates suggests that the population of persistent microquasar systems in the Galaxy is more rare than previously believed. If none of them is galactic, the upper limit to the space density of new Cygnus X-3-like microquasars within 15 kpc would be 1.1\times10^{-12} per cubic pc. A similar upper limit for new LS 5039-like systems within 4 kpc is estimated to be 5.6\times10^{-11} per cubic pc.

LS 5039: A runaway microquasar ejected from the galactic plane

We have compiled optical and radio astrometric data of the microquasar LS 5039 and derived its proper motion. This, together with the distance and radial velocity of the system, allows us to state that this source is escaping from its own regional standard of rest, with a total systemic velocity of about 150 km/s and a component perpendicular to the galactic plane larger than 100 km/s. This is probably the result of an acceleration obtained during the supernova event that created the compact object in this binary system. We have computed the trajectory of LS 5039 in the past, and searched for OB associations and supernova remnants in its path. In particular, we have studied the possible association between LS 5039 and the supernova remnant G016.8-01.1, which, despite our efforts, remains dubious. We have also discovered and studied an HI cavity in the ISM, which could have been created by the stellar wind of LS 5039 or by the progenitor of the compact object in the system. Finally, in the symmetric supernova explosion scenario, we estimate that at least 17 solar masses were lost in order to produce the high eccentricity observed. Such a mass loss could also explain the observed runaway velocity of the microquasar.

EVN+MERLIN observations of microquasar candidates at low galactic latitudes

In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a long-term project focused on the search for new objects of this type. They performed a cross-identification between X-ray and radio catalogs under very restrictive selection criteria for sources with |b|<5 degrees, and obtained a sample of 13 radio-emitting X-ray sources. Follow-up observations of 6 of these sources with the VLA provided accurate coordinates, which were used to discover optical counterparts for all of them. We have observed these six sources with the EVN and MERLIN at 5 GHz. Five of the six objects have been detected and imaged, presenting different morphologies: one source has a two-sided jet, three sources have one-sided jets, and one source is compact. With all the presently available information, we conclude that two of the sources are promising microquasar candidates in our Galaxy.

Proporción de carga asistencial generada por la diabetes mellitus en las consultas de enfermería de atención primaria de salut

Objetivo La mayoría de enfermos con diabetes mellitus tipo 2 (DM2) se controla en atención primaria de salud (APS). La atención y educación proporcionadas por enfermería son clave para controlar la glucemia y prevenir las complicaciones macro y microangiopáticas de la DM. El objetivo de este trabajo es conocer la proporción de carga asistencial atribuible a la DM en consultas de enfermería de APS. Material y método Estudio observacional, analítico y transversal. Durante 2 semanas consecutivas se registraron datos de todos los enfermos que acudieron a 15 consultas de enfermería de APS ubicadas en 14 Áreas Básicas de Salud (ABS) de la provincia de Barcelona. Las variables de estudio fueron: edad, sexo, situación laboral, motivo de consulta, duración de la visita, presencia de DM y, en los enfermos diabéticos, el tipo de tratamiento. La recogida de datos se realizó en 2 períodos. El primero entre noviembre del año 2003 y enero del 2004 y el segundo en abril de 2005. Se realizó un análisis descriptivo de estas variables con un intervalo de confianza del 95% y la asociación entre variables mediante el programa SPSS v.11.1. Resultados Tenía DM el 29% de los pacientes. La DM es el primer motivo de consulta (29,1%), aumenta con la edad y llega al 40% en mayores de 65 años. La duración media de una visita por DM es de 14,59 min, un 30,8% más elevada que la duración media del resto de los problemas de salud. Globalmente, las mujeres consultan más que los varones (56,6%) excepto en DM, curas y hábito tabáquico. Conclusiones La DM es el problema de salud que genera más demanda y consume más tiempo de enfermería en la APS. Esta realidad y el futuro que se prevé con relación al incremento de la prevalencia de DM exigen considerar nuevas estrategias organizativas y formativas, y establecer criterios para mejorar la gestión de recursos y promover estrategias educativas más efectivas.

Proporción de carga asistencial generada por la diabetes mellitus en las consultas de enfermería de atención primaria de salut

Objetivo La mayoría de enfermos con diabetes mellitus tipo 2 (DM2) se controla en atención primaria de salud (APS). La atención y educación proporcionadas por enfermería son clave para controlar la glucemia y prevenir las complicaciones macro y microangiopáticas de la DM. El objetivo de este trabajo es conocer la proporción de carga asistencial atribuible a la DM en consultas de enfermería de APS. Material y método Estudio observacional, analítico y transversal. Durante 2 semanas consecutivas se registraron datos de todos los enfermos que acudieron a 15 consultas de enfermería de APS ubicadas en 14 Áreas Básicas de Salud (ABS) de la provincia de Barcelona. Las variables de estudio fueron: edad, sexo, situación laboral, motivo de consulta, duración de la visita, presencia de DM y, en los enfermos diabéticos, el tipo de tratamiento. La recogida de datos se realizó en 2 períodos. El primero entre noviembre del año 2003 y enero del 2004 y el segundo en abril de 2005. Se realizó un análisis descriptivo de estas variables con un intervalo de confianza del 95% y la asociación entre variables mediante el programa SPSS v.11.1. Resultados Tenía DM el 29% de los pacientes. La DM es el primer motivo de consulta (29,1%), aumenta con la edad y llega al 40% en mayores de 65 años. La duración media de una visita por DM es de 14,59 min, un 30,8% más elevada que la duración media del resto de los problemas de salud. Globalmente, las mujeres consultan más que los varones (56,6%) excepto en DM, curas y hábito tabáquico. Conclusiones La DM es el problema de salud que genera más demanda y consume más tiempo de enfermería en la APS. Esta realidad y el futuro que se prevé con relación al incremento de la prevalencia de DM exigen considerar nuevas estrategias organizativas y formativas, y establecer criterios para mejorar la gestión de recursos y promover estrategias educativas más efectivas.

Dietary resveratrol prevents alzheimer's markers and increases life span in SAMP8

Resveratrol is a polyphenol that is mainly found in grapes and red wine and has been reported to be a caloric restriction (CR) mimetic driven by Sirtuin 1 (SIRT1) activation. Resveratrol increases metabolic rate, insulin sensitivity, mitochondrial biogenesis and physical endurance, and reduces fat accumulation in mice. In addition, resveratrol may be a powerful agent to prevent age-associated neurodegeneration and to improve cognitive deficits in Alzheimer's disease (AD). Moreover, different findings support the view that longevity in mice could be promoted by CR. In this study, we examined the role of dietary resveratrol in SAMP8 mice, a model of age-related AD. We found that resveratrol supplements increased mean life expectancy and maximal life span in SAMP8 and in their control, the related strain SAMR1. In addition, we examined the resveratrol-mediated neuroprotective effects on several specific hallmarks of AD. We found that long-term dietary resveratrol activates AMPK pathways and pro-survival routes such as SIRT1 in vivo. It also reduces cognitive impairment and has a neuroprotective role, decreasing the amyloid burden and reducing tau hyperphosphorylation.

Dietary resveratrol prevents alzheimer's markers and increases life span in SAMP8

Resveratrol is a polyphenol that is mainly found in grapes and red wine and has been reported to be a caloric restriction (CR) mimetic driven by Sirtuin 1 (SIRT1) activation. Resveratrol increases metabolic rate, insulin sensitivity, mitochondrial biogenesis and physical endurance, and reduces fat accumulation in mice. In addition, resveratrol may be a powerful agent to prevent age-associated neurodegeneration and to improve cognitive deficits in Alzheimer's disease (AD). Moreover, different findings support the view that longevity in mice could be promoted by CR. In this study, we examined the role of dietary resveratrol in SAMP8 mice, a model of age-related AD. We found that resveratrol supplements increased mean life expectancy and maximal life span in SAMP8 and in their control, the related strain SAMR1. In addition, we examined the resveratrol-mediated neuroprotective effects on several specific hallmarks of AD. We found that long-term dietary resveratrol activates AMPK pathways and pro-survival routes such as SIRT1 in vivo. It also reduces cognitive impairment and has a neuroprotective role, decreasing the amyloid burden and reducing tau hyperphosphorylation.

Maria Furuhjelms Notebok

Soitinnus: piano.