Use of Diethanolamine to Obain Cellulosics Pulps from Solid Fraction of Hydrothermal Treatment of Rice Straw

We assessed the potential of the solid residue from ahydrothermal treatment of rice straw as an alternative raw material for obtaining cellulose pulp. To this end, we examined the influence of operational variables in the diethanolamine pulping of this material on the properties of the cellulose pulp obtained and of paper sheets made from it.Using a central composite factor design and fitting the results to a polynomial model allowed us to establish equations relating the dependent variables to the independent ones with errors less than 8% in all cases except for burst index (27%).The optimum conditions with a view to saving reagents, heating energy and immobilized capital were found to be a diethanolamine concentration of 70%, a temperature of 162.5 ºC, a cooking time of 60 min and a liquid/solid ratio of 8. These conditions provide paper sheets with physical properties that depart by less than 8% from their optimum values, and a pulp yield and Kappa number differing by less than 14% from their best levels.We compared the results obtained in the diethanolaminepulping of the solid fraction from the hydrothermal treatmentof rice straw with those for kraft and diethanolaminepulp from eucalyptus and pine wood, and found the propertiesof the former to fall in between those for the latter two

Capacidad aeróbica, felicidad y satisfacción con la vida en adolescentes españoles

Analizar la asociación entre capacidad aeróbica, felicidad subjetiva y satisfacción con la vida en adolescentes. Método: Participaron 388 adolescentes (207 mujeres) de 12-18 años de edad. La capacidad aeróbica se evaluó mediante el test de 20 metros de ida y vuelta. La felicidad subjetiva y la satisfacción con la vida se evaluaron mediante las escalas Subjective Happiness Scale y Satisfaction With Life Scale, respectivamente. Se midió el peso y la talla de los adolescentes y se calculó el índice de masa corporal (IMC). Los adolescentes indicaron el nivel de estudios de la madre. Resultados: Los análisis de regresión lineal mostraron que la capacidad aeróbica se asocia positivamente con felicidad subjetiva (ß no estandarizada = .09 ± .03, r = .128, p = .013) y satisfacción con la vida (ß no estandarizada = .31 ± .13, r = .118, p = .022), independientemente del sexo, IMC y estudios de la madre. Conclusión: Los resultados de este estudio sugieren que los adolescentes que tienen una mejor capacidad aeróbica también son más felices y tienen una mayor satisfacción con la vida. Hacen falta estudios de intervención para corroborar si un programa dirigido a la mejora de la capacidad aeróbica puede también influir en el nivel de felicidad y satisfacción vital en adolescentes.To analyse the interrelations among cardiorespiratory fitness, subjective happiness and satisfaction with life in adolescents. Method: The study was based on a total of 388 Spanish adolescents (207 females) aged 12-18. Cardiorespiratory fitness was assessed by means of the 20-metre shuttle run test. Subjective happiness and satisfaction with life were assessed using the Subjective Happiness Scale and Satisfaction with Life Scale respectively. The adolescents' height and weight were measured and their body mass index (BMI) calculated. They were asked to report the educational level of the mother. Results: The linear regression analysis showed that cardiorespiratory fitness was positively associated with subjective happiness (ß non standardized = .09 ± .03, r = .128, p = .013) and satisfaction with life (ß non standardized = .31 ± .13, r = .128, p = .022), regardless of the subjects' sex, BMI, and educational level of the mother. Conclusion: These findings suggest that adolescents with a good level of cardiorespiratory fitness are happier and more satisfied with life. Intervention studies are needed to confirm whether an intervention programme aimed at improving aerobic performance might also lead to improvements in adolescents' level of happiness and satisfaction with life

Deterioration of an Etruscan tomb by bacteria from the order Rhizobiales

7 páginas, 4 figuras, 29 referencias.The Etruscan civilisation originated in the Villanovan Iron Age in the ninth century BC and was absorbed by Rome in the first century BC. Etruscan tombs, many of which are subterranean, are one of the best representations of this culture. The principal importance of these tombs, however, lies in the wall paintings and in the tradition of rich burial, which was unique in the Mediterranean Basin, with the exception of Egypt. Relatively little information is available concerning the biodeterioration of Etruscan tombs, which is caused by a colonisation that covers the paintings with white, circular to irregular aggregates of bacteria or biofilms that tend to connect each other. Thus, these colonisations sometimes cover extensive surfaces. Here we show that the colonisation of paintings in Tomba del Colle is primarily due to bacteria of the order Rhizobiales (Alphaproteobacteria), which were likely influenced by the neighbouring rhizosphere community and the availability of nutrients from root exudates.This work was funded through the projects CGL2010-17183, 201030E011 and Consolider 2007-00058. M.D.H. was supported by a JAE Research Fellowship from CSIC, and S.C. was supported by a Juan de la Cierva contract.Peer reviewe

SHARDS: Constraints on the dust attenuation law of star-forming galaxies at z~2

We make use of SHARDS, an ultra-deep (<26.5AB) galaxy survey that provides optical photo-spectra at resolution R~50, via medium band filters (FWHM~150A). This dataset is combined with ancillary optical and NIR fluxes to constrain the dust attenuation law in the rest-frame NUV region of star-forming galaxies within the redshift window 1.5<z<3. We focus on the NUV bump strength (B) and the total-to-selective extinction ratio (Rv), targeting a sample of 1,753 galaxies. By comparing the data with a set of population synthesis models coupled to a parametric dust attenuation law, we constrain Rv and B, as well as the colour excess, E(B-V). We find a correlation between Rv and B, that can be interpreted either as a result of the grain size distribution, or a variation of the dust geometry among galaxies. According to the former, small dust grains are associated with a stronger NUV bump. The latter would lead to a range of clumpiness in the distribution of dust within the interstellar medium of star-forming galaxies. The observed wide range of NUV bump strengths can lead to a systematic in the interpretation of the UV slope ($\beta$) typically used to characterize the dust content. In this study we quantify these variations, concluding that the effects are $\Delta\beta$~0.4.Comment: 13 pages, 11+2 figures, 3 tables. MNRAS, in pres

Efectividad del consejo médico a pacientes alcohólicos y bebedores excesivos atendidos en consultas de atención primaria

ObjetivoComprobar la efectividad del consejo médico antialcohólico que se da en las consultas de atención primaria.DiseñoEstudio cuasi-experimental de tipo «antes-después», abierto, multicéntrico.EmplazamientoCatorce consultas médicas de atención primaria (7 rurales y 7 urbanas) de la provincia de Córdoba (España).ParticipantesUn total de 306 pacientes de ambos sexos, captados mediante búsqueda de casos, que presentaban un consumo de alcohol ≥ 35 (varones) y 21 (mujeres) U a la semana, y/o síndrome de dependencia alcohólica (SDA) (MALTS-O ≥ 11).IntervencionesA todos se les ofreció consejo médico breve antialcohólico y se les hizo un seguimiento para valoración de su estado a los 3 meses, 1 y 2 años.Mediciones principalesLa variable de respuesta fue la suma del consumo autorreferido, más valores normales de GGT, y la confirmación del familiar. El análisis del estudio fue por «intención de tratar».ResultadosDe los 306 pacientes incluidos, en un 95,1% de los casos se trataba de varones y un 78,4% presentaba SDA. Al cabo de 2 años, el 38,89% (IC del 95%, 32,2-44,3%) había alcanzado el objetivo terapéutico: un 23,85% se encontraba en abstinencia total y el 15,0% presentaba un consumo moderado de alcohol, por debajo del límite de riesgo. El comienzo del consumo excesivo antes de los 16 años (odds ratio [OR], 3,0885), vivir en un barrio marginal (OR, 3,2103), consumir tabaco (OR, 1,7187) y un test de CAGE positivo (OR, 1,9949) se asociaron al fracaso de la intervención (p < 0,05).ConclusionesSe demuestra la alta efectividad del consejo antialcohólico impartido por el médico de familia en condiciones habituales de consulta, tanto en bebedores excesivos como en aquellos con SDA.AimTo determine the effectiveness of medical counseling for alcohol abuse, when it is provided in primary care centers.DesignQuasi-experimental, open, multicenter before-after study.Setting14 primary care physician's practices (7 rural, 7 urban) in the province of Córdoba (Spain).Participants306 patients of both sexes, recruited with a case-finding strategy, who consumed ≥35 (men) or ≥21 (women) IU per week, or who had alcohol dependence syndrome (ADS) (MALTS score O≥11).InterventionsAll patients were offered brief counseling to reduce drinking, and all were followed to evaluate their status 3 months, 1 year and 2 years later.Main measuresThe response variable was selfreported alcohol consumption together with normal GGT values or confirmation of alcohol consumption by a relative. The results were subjected to intention-to-treat analysis.ResultsOf the 306 patients included in the study, 95.1% were men and 78.4% had ADS. After 2 years 38.89% (95% CI, 32.2%-44.3%) had attained their treatment goal: 23.85% were in complete abstinence, and 15.0% consumed moderate amounts of alcohol below the limit considered to indicate risk. Starting excessive consumption at less than 16 years of age (odds ratio [OR], 3.0885), living in a slum (OR, 3.2103), smoking (OR, 1.7187), and a positive CAGE test (OR, 1.9949) were associated with failure of the intervention (P<.05).ConclusionsCounseling provided by the family doctor was highly effective under the usual conditions of general practice, both for patients with excessive alcohol consumption and for patients with con ADS

Spectroscopic evidence of distinct stellar populations in the counter-rotating stellar disks of NGC 3593 and NGC 4550

We present the results of integral-field spectroscopic observations of the two disk galaxies NGC 3593 and NGC 4550 obtained with VIMOS/VLT. Both galaxies are known to host 2 counter-rotating stellar disks, with the ionized gas co-rotating with one of them. We measured in each galaxy the ionized gas kinematics and metallicity, and the surface brightness, kinematics, mass surface density, and the stellar populations of the 2 stellar components to constrain the formation scenario of these peculiar galaxies. We applied a novel spectroscopic decomposition technique to both galaxies, to separate the relative contribution of the 2 counter-rotating stellar and one ionized-gas components to the observed spectrum. We measured the kinematics and the line strengths of the Lick indices of the 2 counter-rotating stellar components. We modeled the data of each stellar component with single stellar population models that account for the alpha/Fe overabundance. In both galaxies we successfully separated the main from the secondary stellar component that is less massive and rotates in the same direction of the ionized-gas component. The 2 stellar components have exponential surface-brightness profiles. In both galaxies, the two counter-rotating stellar components have different stellar populations: the secondary stellar disk is younger, more metal poor, and more alpha-enhanced than the main galaxy stellar disk. Our findings rule out an internal origin of the secondary stellar component and favor a scenario where it formed from gas accreted on retrograde orbits from the environment fueling an in situ outside-in rapid star formation. The event occurred ~ 2 Gyr ago in NGC 3593, and ~ 7 Gyr ago in NGC 4550. The binary galaxy merger scenario cannot be ruled out, and a larger sample is required to statistically determine which is the most efficient mechanism to build counter-rotating stellar disks (abridged).Comment: 13 pages, 9 figures, accepted for publication in Astronomy and Astrophysic

Assessing the internal uppermost crustal structure of the central pyrenees by gravity-constrained cross sections

The Pyrenees constitutes an exceptional example of an Alpine orogenic belt characterized by basement thrust sheets involving Paleozoic rocks and Mesozoic and Cenozoic cover units detached on the Triassic evaporites, the main décollement level. This work is located in the Central Pyrenees, where gravity data help to better constrain the internal architecture of the upper crust of the southern half of the Axial Zone and the northern part of the South Pyrenean Zone, a key area to understand the orogenic evolution of the chain. Previous and new gravity, petrophysical and geological data have been used to obtain the Bouguer and residual anomaly maps of the study area and six serial gravity-constrained cross sections perpendicular to the main structural trend. The residual anomaly map shows a good correlation between basement units involved in thrust sheets of the study area and gravity highs whereas negative anomalies are interpreted to correspond with Mesozoic/Cenozoic basins, Triassic evaporites, Late Variscan igneous bodies, and Ordovician gneisses. The six gravity-constrained cross sections highlight strong along-strike variations on the gravity signal due to lateral differences of the superficial and subsurface occurrence of Triassic evaporites, different geometry at depth of the Late Variscan igneous bodies outcropping in the study area, and geometric lateral variations of the basement thrust sheets and their relationship with the Mesozoic-Cenozoic units.This work was funded by projects CGL2017-84901-C2-2-P funded by MCIN/AEI/10.13039/501100011033 and “ERDF A way of making Europe”, PID2020-114273GB-C22 funded by MCIN/AEI/10.13039/501100011033 from the Spanish Ministry of Science and Innovation, and "Severo Ochoa” extraordinary grants for excellence IGME-CSIC (AECEX2021).Peer reviewe

The bright galaxy population of five medium redshift clusters. II. Quantitative Galaxy Morphology

Aims: Following the study already presented in our previous paper, based on the Nordic Optical Telescope (NOT) sample, which consists of five clusters of galaxies within the redshift range 0.18 $\leq$ z $\leq$ 0.25, imaged in the central 0.5-2 Mpc in very good seeing conditions, we have studied the quantitative morphology of their bright galaxy population Methods: We have analyzed the surface brightness profiles of the galaxy population in those clusters. Previously, we have performed simulations in order to check the reliability of the fits. We have also derived a quantitative morphological classification. Results: The structural parameters derived from these analysis have been analyzed. We have obtained that the structural parameters of E/S0 galaxies are similar to those showed by galaxies in low redshift clusters. However, the disc scales are different. In particular, the scales of the discs of galaxies at medium redshift clusters are statistically different than those located in similar galaxies in the Coma cluster. But, the scales of the discs of galaxies in medium redshift clusters are similar to nearby field galaxies. Conclusions: The results suggest that the evolution of the disc component of galaxies in clusters is faster than in field ones. Mechanisms like galaxy harassment showing timescales of $\sim 1$Gyr could be the responsible of this disc scale evolution. This indicates that spiral galaxies in clusters have suffered a strong evolution in the last 2.5 Gyr or that Coma is in some way anomalous.Comment: 13 pages, 10 figures, Accepted for publication in A&

The Effect of Patients’ Met Expectations on Consultation Outcomes. A Study with Family Medicine Residents

OBJECTIVES: To know the patients’ expectations and the fulfillment of these at family medicine consultations by resident doctors and to assess their effect on some consultation outcomes. DESIGN: A prospective cohort study. PARTICIPANTS: Patients attending family medicine consultations held by 38 resident doctors: 1,301 eligible patients, 702 filled in all questionnaires. MEASUREMENTS: Before each visit, the patients’ expectations about that particular consultation were registered. Right after the visit was over, their perception of several aspects of the communicative interaction with the doctor was measured. Later, patients were interviewed on the phone to know how their expectations had been fulfilled, how satisfied they were about the consultation, how they had followed the doctor’s suggestions, if they were going to seek further care for the same cause later, and the evolution of their clinical problem. Logistic regression was the main analysis used. RESULTS: The most common expectations were the doctor showing interest and listening (30.5%), getting some information about the diagnosis (16.3%), and sharing problems and doubts (11.1%). The rate of main expectations that were met was 76.5%. Satisfaction with the encounter was associated with the clinical evolution [odds ratio (OR) 2.23; confidence interval (CI): 1.32–3.75], and the fulfilling of the patients’ main or two main expectations was significantly related to all the measured outcomes (satisfaction OR 3.51, CI: 1.73–7.8; adherence OR 1.80, CI: 1.11–2.92; clinical evolution OR 1.54, CI: 1.01–2.35; and seeking further care later OR 0.54, CI:0.36–0.81) CONCLUSIONS: Patients prioritize expectations of a more general sort when they attend primary care consultations and residents fulfill these acceptably. The fulfillment of expectations seems to affect the studied outcomes more than other factors