Cardiopatías congénitas en el perro : conducto arterioso persistente, estenosis pulmonar y estenosis aórtica

En el presente artículo se describen los hallazgos clínicos, radiológicos, electrocardiográficos y ecográficos de las principales cardiopatías congénitas en el perro de acuerdo con una serie de casos clínicosClinical signs and radiological, electro and echocardiographic findings of the main congenital heart diseases in the dog are described in this paper based on c1inicalcases

Multi-zone non-thermal radiative model for stellar bowshocks

Context. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non-thermal radio emission has been detected so far only from the bowshock of BD+43°3654, whereas the detection of non-thermal radiation from these bowshocks at high energies remains elusive. Aims. We aim at characterising in detail the radio, X-ray, and γ-ray emission from stellar bowshocks accounting for the structure of the region of interaction between the stellar wind and its environment. Methods. We develop a broadband-radiative, multi-zone model for stellar bowshocks that takes into account the spatial structure of the emitting region and the observational constraints. The model predicts the evolution and the emission of the relativistic particles accelerated and streaming together with the shocked flow. Results. We present broadband non-thermal spectral energy distributions for different scenarios, synthetic radio-cm synchrotron maps that reproduce the morphology of BD+43°3654, and updated predictions in X-ray and γ-ray energy ranges. We also compare the results of the multi-zone model applied in this work with those of a refined one-zone model. Conclusions. A multi-zone model provides better constraints than a one-zone model on the relevant parameters, namely the magnetic field intensity and the amount of energy deposited in non-thermal particles. However, one-zone models can be improved by carefully characterising the intensity of the IR dust photon field and the escape rate of the plasma from the shocked region. Finally, comparing observed radio maps with those obtained from a multi-zone model enables constraints to be obtained on the direction of stellar motion with respect to the observer

Vítreo primario hiperplásico persistente y anomalías asociadas en un Husky siberiano

Se describe el caso clínico de una perra Husky siberiano que acudio a consulta para una evaluacion ocular porque el ojo derecho mostraba aspecto blanquecino. El diagnostico de vitreo primario hiperplastico persistente se efectuo mediante ultrasonografia bidimensional y Doppler color

Regional-scale vegetation heterogeneity in northeastern Patagonia: Environmental and spatial components

Our aim was to describe vegetation heterogeneity at a regional scale in northeastern Patagonia and to identify the environmental variables associated to it. The study area encompasses 13 144 km2 and is characterized by a mixture of species typical of Patagonian steppes and Monte Desert. We performed 48 vegetation relevés, which were randomly assigned to a training set and to a validation set (32 and 16 relevés, respectively). Training set was subjected to cluster analysis, which allowed the identification of two plant communities one related to Patagonian steppes and another to the Monte desert. We derived 3 attributes of the seasonal curve of the NDVI as indicators of ecosystem function: the seasonal amplitude (SA), the date of the maximum (DOM), and the large seasonal integral (LSI). We explored the relationship between NDVI attributes and communities by classification tree analysis. LSI was the strongest predictor among NDVI attributes, separating both communities without misclassification errors. Patagonian steppes occupy areas with higher LSI. The partial RDA analysis explained 38.1% of total data variation, of which 16.5% was ascribed to environment, 7.9% to space, and 13.7% to spatial component of environment. Patagonian steppes are closer to the coast, in areas exhibiting higher annual precipitation and lower annual temperature range than Monte deserts. Our results indicate the occurrence of two plant communities in the study area and highlight the significance of climatic variables to explain their spatial distribution. As most scenarios of future climate predict greater annual thermal amplitude in the study area, the limit between both communities could be displaced eastward

Synchrotron radiation and absence of linear polarization in the colliding wind binary WR 146

Context. Several massive early-type binaries exhibit non-thermal emission which has been attributed to synchrotron radiation from particles accelerated by diffusive shock acceleration (DSA) in the wind-collision region (WCR). If the magnetic field in the strong shocks is ordered, its component parallel to the shock front should be enhanced, and the resultant synchrotron radiation would be polarized. However, such polarization has never been measured. Aims. We aim to determine the percentage of linearly polarized emission from the well-known non-thermal radio emitter WR 146, a WC6+O8 system. Methods. We performed spatially-unresolved radio continuum observations of WR 146 at 5 cm and 20 cm with the Karl G. Jansky Very Large Array. We constructed a numerical model to investigate a scenario where particles are accelerated by turbulent magnetic reconnection (MR), and we performed a quantitative analysis of possible depolarization effects. Results. No linearly polarized radio emission was detected. The data constrain the fractional linear polarization to less than 0.6% between 1 to 8 GHz. This is compatible with a high level of turbulence and a dominant random component in the magnetic field. In this case the relativistic particles could be produced by turbulent magnetic reconnection. In order for this scenario to satisfy the required non-thermal energy budget, the strength of the magnetic field in the WCR must be as high as ∼ 150 mG. However, if the magnetic field is ordered and DSA is ongoing, then a combination of internal and external Faraday rotation could equally account for the depolarization of the emission. Conclusions. The absence of polarization could be caused by a highly turbulent magnetic field, other depolarization mechanisms such as Faraday rotation in the stellar wind, or a combination of these processes. It is not clear whether it is possible to develop the high level of turbulence and strong magnetic fields required for efficient MR in a long-period binary such as WR 146. This scenario might also have trouble explaining the low-frequency cutoff in the spectrum. We therefore favor a scenario where particles are accelerated through DSA and the depolarization is produced by mechanisms other than a large ratio between random to regular magnetic fields.Facultad de Ciencias Astronómicas y GeofísicasInstituto Argentino de Radioastronomí

Disautonomía felina

En el presente trabajo, se efectúa una revisión completa del síndrome disautonomía felina, así como la descripción de un caso clínico correspondiente a un gato macho de 11 meses de edad, junto con los medios de diagnóstico utilizado.At the present research a review ol the dysautonomia feline syndrome is included with the description of a clinical case in a male cat of 11 months of age

Bloqueo atrioventricular completo en un perro : tratamiento mediante la implantación de un marcapasos endovenosos permanente

Una perra Labrador Retriever presentaba una historia de síncopes, fatiga e intolerancia al ejercicio debida a un bloqueo atrioventricular completo. Debido a que no respondía a la terapia médica (terbutalina, teofilina y posteriormente atropina), fue remitida al Hospital Clínico Veterinario de la Universidad de Murcia con el fin de considerar la implantación de un marcapasos. Las radiografías de tórax mostraron aumento global de la silueta cardiaca y la ecocardiografía puso de manifiesto, además, ligera regurgitación de válvulasatrioventriculares. Se le implantó un marcapasos endovenoso permanente unipolar con modo VVI bajo anestesia general, guiando el cable hacia el ventrículo derecho mediante fluoroscopia con amplificador de imagen. Ocho meses después de la implantación, no se han producido complicaciones y el marcapasos funciona según los parámetros programados.

Secondary hyperparathyroidism in HIV-infected patients: relationship with bone remodeling and response to vitamin D supplementation

Purpose of the study: Secondary hyperparathyroidism (SH) is frequent in HIV-infected patients. However, the causes and consequences are not well established. The aim of our study was to determine the relationship between parathyroid hormone (PTH), vitamin D and bone mineral density (BMD) in HIV-infected patients, and the effect of vitamin D replacement on PTH levels. Methods: Prospective study of 506 patients with at least two sequential serum determinations of PTH and 25-hydroxyvitamin D levels. In all cases, a bone dual X-ray absorptiometry (DEXA) was performed at inclusion. Hyperparathyroidism was defined as a PTH level above 65 pg/ml. Summary of results: Mean age was 44 yrs (24–78), and 75% were male. Mean BMI was 23.7 (17.97–33.11), and only 3% were of black race. Median nadir CD4+ was 200 cells/µL (9–499), and median time of HIV infection was 15.3 yrs (1.7–25.2). At inclusion, 488 patients (86%) were on HAART (31% TDF+PI, 44% TDF+NNRTI, 25% non-TDF based regimen) for a median of 929.5 days (154–1969), and 40% were HCV-coinfected. Median eGFR was 97.9 ml/min (62.14–134.08). Overall, mean serum PTH was 56.3 pg/mL (27.2–95.07). SH was observed in 27% of cases, with a marked influence of seasonality (from 44% in January to 10% in August). Mean levels of vitamin D were 17.45 ng/mL (7.6–40.78), with 16% below 10 ng/ml, 59%<20 ng/ml (deficiency), 85%<30 ng/ml (insufficiency). SH was related to vitamin D deficiency (relative risk, RR, 2.44), age (RR 1.04 per year), and a higher decrease in eGFR (RR 1.03 per ml/min), after adjustment by season, antiretroviral therapy, GFR at baseline, and HCV coinfection. DEXA scan showed 18% osteoporosis and 54% osteopenia, and there was an inverse correlation between PTH levels and T and Z score in femoral neck (r=−0.14, p<0.01), higher in those patients below 40 yrs. Vitamin D supplementation in 181 patients produced a significant decrease in serum PTH (57.2 if not treated vs 50.5 pg/ml, p=0.02, 23% continues with SH) and the only factor associated with lack of response was persistent vitamin D deficiency. Conclusion: SH is relatively frequent in HIV patients, in close relation with vitamin D deficiency. It is associated with bone resorption, especially in the femoral neck. The use of vitamin D supplementation improves SH when levels above 20 ng/ml are achieved

New Insights into the HII Region G18.88-0.49: Hub-Filament System and Accreting Filaments

We present an analysis of multiwavelength observations of an area of 0.°27 × 0.°27 around the Galactic H ii region G18.88-0.49, which is powered by an O-type star (age ∼ 105 yr). The Herschel column density map reveals a shell-like feature of extension ∼12 pc × 7 pc and mass ∼2.9 × 104 M o˙ around the H ii region; its existence is further confirmed by the distribution of molecular (12CO, 13CO, C18O, and NH3) gas at [60, 70] km s-1. Four subregions are studied toward this shell-like feature and show a mass range of ∼0.8-10.5 × 103 M o˙. These subregions associated with dense gas are dominated by nonthermal pressure and supersonic nonthermal motions. The shell-like feature is associated with the H ii region, Class I protostars, and a massive protostar candidate, illustrating the ongoing early phases of star formation (including massive stars). The massive protostar is found toward the position of the 6.7 GHz methanol maser, and is associated with outflow activity. Five parsec-scale filaments are identified in the column density and molecular maps and appear to be radially directed to the dense parts of the shell-like feature. This configuration is referred to as a "hub-filament"system. Significant velocity gradients (0.8-1.8 km s-1 pc-1) are observed along each filament, suggesting that the molecular gas flows toward the central hub along the filaments. Overall, our observational findings favor a global nonisotropic collapse scenario as discussed in Motte et al., which can explain the observed morphology and star formation in and around G18.88-0.49.Fil: Dewangan, L. K.. Physical Research Laboratory India; IndiaFil: Ojha, D. K.. International Centre Of Theoretical Science. Tata Institute Of Fundamental Research; EspañaFil: Sharma, Saurabh. Aryabhatta Research Institute Of Observational Sciences; IndiaFil: del Palacio, Santiago. Universidad Nacional de La Plata; Argentina. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Bhadari, N. K.. Indian Institute Of Technology Gandhinagar; India. Physical Research Laboratory India; IndiaFil: Das, A.. University Of Hyderabad; Indi