Ammonia observations of the nearby molecular cloud MBM 12

We present NH3(1,1) and NH3(2,2) observations of MBM 12, the closest known molecular cloud (65 pc distance), aimed to find evidence for on-going star formation processes. No local temperature (with a T_rot upper limit of 12 K) nor linewidth enhancement is found, which suggests that the area of the cloud we mapped (~ 15' size) is not currently forming stars. Therefore, this close ``starless'' molecular gas region is an ideal laboratory to study the physical conditions preceding new star formation. A radio continuum source was found in Very Large Array archive data, close but outside the NH3 emission. This source is likely to be a background object.Comment: 8 pages, 3 figures, accepted by MNRA

Evidence Against the Sciama Model of Radiative Decay of Massive Neutrinos

We report on spectral observations of the night sky in the band around 900 angstroms where the emission line in the Sciama model of radiatively decaying massive neutrinos would be present. The data were obtained with a high resolution, high sensitivity spectrometer flown on the Spanish MINISAT satellite. The observed emission is far less intense than that expected in the Sciama model.Comment: 9 pages, accepted to Ap

Far Ultraviolet Absolute Flux of alpha Virginis

We present the far ultraviolet spectrum of alpha Virginis taken with EURD spectrograph on-board MINISAT-01. The spectral range covered is from ~900 to 1080 A with 5 A spectral resolution. We have fitted Kurucz models to IUE spectra of alpha Vir and compared the extension of the model to our wavelengths with EURD data. This comparison shows that EURD fluxes are consistent with the prediction of the model within 20-30%, depending on the reddening assumed. EURD fluxes are consistent with Voyager observations but are ~60% higher than most previous rocket observations of alpha Vir.Comment: 13 pages, 4 figures. Submitted to The Astrophysical Journa

Far Ultraviolet Spectra of B Stars near the Ecliptic

Spectra of B stars in the wavelength range of 911-1100 A have been obtained with the EURD spectrograph onboard the Spanish satellite MINISAT-01 with ~5 A spectral resolution. IUE spectra of the same stars have been used to normalize Kurucz models to the distance, reddening and spectral type of the corresponding star. The comparison of 8 main-sequence stars studied in detail (alpha Vir, epsilon Tau, lambda Tau, tau Tau, alpha Leo, zeta Lib, theta Oph, and sigma Sgr) shows agreement with Kurucz models, but observed fluxes are 10-40% higher than the models in most cases. The difference in flux between observations and models is higher in the wavelength range between Lyman alpha and Lyman beta. We suggest that Kurucz models underestimate the FUV flux of main-sequence B stars between these two Lyman lines. Computation of flux distributions of line-blanketed model atmospheres including non-LTE effects suggests that this flux underestimate could be due to departures from LTE, although other causes cannot be ruled out. We found the common assumption of solar metallicity for young disk stars should be made with care, since small deviations can have a significant impact on FUV model fluxes. Two peculiar stars (rho Leo and epsilon Aqr), and two emission line stars (epsilon Cap and pi Aqr) were also studied. Of these, only epsilon Aqr has a flux in agreement with the models. The rest have strong variability in the IUE range and/or uncertain reddening, which makes the comparison with models difficult.Comment: 25 pages, 6 figures, to be published in The Astrophysical Journa

Modificaciones de la fibrilación ventricular y de la capacidad de captura inducidas por una lesión lineal con radiofrecuencia

[EN] Introduction and objectives: An analysis was made of the effects of a radiofrequency-induced linear lesion during ventricular fibrillation and the capacity to capture myocardium through high-frequency pacing. Methods: Using multiple epicardial electrodes, ventricular fibrillation was recorded in 22 isolated perfused rabbit hearts, analyzing the activation maps upon applying trains of stimuli at 3 different frequencies close to that of the arrhythmia: a) at baseline; b) after radio-frequency ablation to induce a lesion of the left ventricular free wall (length=10 [1] mm), and c) after lengthening the lesion (length=23 [2] mm). Results: Following lesion induction, the regularity of the recorded signals decreased and significant variations in the direction of the activation fronts were observed. On lengthening the lesion, there was a slight increase in the episodes with at least 3 consecutive captures when pacing at cycles 10% longer than the arrhythmia (baseline: 0.6 [0.7]; initial lesion: 1 [1] no significant differences; lengthened lesion: 3 [2.8]; P<.001), while a decrease was observed in those obtained upon pacing at cycles 10% shorter than the arrhythmia. Conclusions: The radio-frequency -induced lesion increases the heterogeneity of myocardial activation during ventricular fibrillation and modifies arrival of the activation fronts in the adjacent zones. High-frequency pacing during ventricular fibrillation produces occasional captures during at least 3 consecutive stimuli. The lengthened lesion in turn slightly increases capture capacity when using cycles slightly longer than the arrhythmia. (C) 2011 Sociedad Espanola de Cardiologia. Published by Elsevier Espana, S.L. All rights reserved.[ES] Introducción y objetivos Analizar los efectos, en la fibrilación ventricular y en la capacidad de capturar al miocardio mediante estimulación a frecuencias rápidas, de una lesión lineal producida con radiofrecuencia. Métodos En 22 corazones de conejo aislados y perfundidos, se utilizaron electrodos múltiples epicárdicos para registrar la fibrilación ventricular. Se analizaron los mapas de activación al aplicar trenes de estímulos a tres frecuencias distintas, cercanas a las de la arritmia, en tres situaciones: a) basalmente, b) tras producir con radiofrecuencia una lesión en la pared libre del ventrículo izquierdo (longitud, 10 ± 1 mm), y c) tras ampliar su extensión (longitud, 23 ± 2 mm). Resultados Tras la lesión, se observó una disminución de la regularidad de las señales registradas y variaciones significativas en la dirección de los frentes de activación. Con la lesión ampliada, se incrementaron ligeramente los episodios con al menos tres capturas consecutivas al estimular con ciclos un 10% más largos que los de la arritmia (basal, 0,6 ± 0,7; lesión inicial, 1 ± 1, diferencias no significativas; lesión ampliada, 3 ± 2,8; p < 0,001), mientras que se redujeron los obtenidos al estimular con ciclos un 10% más cortos que los de la arritmia. Conclusiones La lesión efectuada con radiofrecuencia aumenta la heterogeneidad de la activación miocárdica durante la fibrilación ventricular y modifica la llegada de los frentes de activación a las zonas adyacentes. La estimulación durante la fibrilación ventricular a frecuencias rápidas provoca capturas ocasionales durante al menos tres estímulos consecutivos. La lesión ampliada incrementa ligeramente la capacidad de captura al utilizar ciclos ligeramente más largos que los de la fibrilación ventricular.This study was funded by research grants from the Instituto de Salud Carlos III FIS PI06/0758-PS09/02417 and RETIC REDINSCOR RD06/0003/0010, from the Generalitat Valenciana PROMETEO 2010/093, and from the Sociedad Espanola de Cardiologia.Chorro, FJ.; Pelechano Ribes, F.; Trapero, I.; Ibañez Catala, X.; Such-Miquel, L.; Tormos Ferrando, Á.; Guerrero, J.... (2012). Modifications in Ventricular Fibrillation and Capture Capacity Induced by a Linear Radiofrequency Lesion. Revista Española de Cardiología. 65(2):143-151. https://doi.org/10.1016/j.rec.2011.09.016S14315165