Discovery of "Warm Dust" galaxies in clusters at z ~ 0.3: evidence for stripping of cool dust in the dense environment?

Using far-infrared imaging from the "Herschel Lensing Survey," we derive dust properties of spectroscopically confirmed cluster member galaxies within two massive systems at z ~ 0.3: the merging Bullet Cluster and the more relaxed MS2137.3-2353. Most star-forming cluster sources (~90%) have characteristic dust temperatures similar to local field galaxies of comparable infrared (IR) luminosity (T_dust ~ 30 K). Several sub-luminous infrared galaxy (LIRG; L_IR < 10^11 L_☉) Bullet Cluster members are much warmer (T_dust > 37 K) with far-infrared spectral energy distribution (SED) shapes resembling LIRG-type local templates. X-ray and mid-infrared data suggest that obscured active galactic nuclei do not contribute significantly to the infrared flux of these "warm dust" galaxies. Sources of comparable IR luminosity and dust temperature are not observed in the relaxed cluster MS2137, although the significance is too low to speculate on an origin involving recent cluster merging. "Warm dust" galaxies are, however, statistically rarer in field samples (>3σ), indicating that the responsible mechanism may relate to the dense environment. The spatial distribution of these sources is similar to the whole far-infrared bright population, i.e., preferentially located in the cluster periphery, although the galaxy hosts tend toward lower stellar masses (M_* < 10^10 M_☉). We propose dust stripping and heating processes which could be responsible for the unusually warm characteristic dust temperatures. A normal star-forming galaxy would need 30%-50% of its dust removed (preferentially stripped from the outer reaches, where dust is typically cooler) to recover an SED similar to a "warm dust" galaxy. These progenitors would not require a higher IR luminosity or dust mass than the currently observed normal star-forming population.

Farmacocinética de oxitetraciclina en dosificación oral múltiple en cerdos. Análisis PK-PD

La oxitetraciclina, antibiótico de amplio uso en medicina veterinaria, pertenece al grupo de las tetraciclinas. Inhibe la síntesis de proteínas en la bacteria a nivel ribosomal. La oxitetraciclina presenta principalmente una acción bacteriostática frente a bacterias Gram-positivas y Gram-negativas, así como también frente a otros microorganismos tales como micoplasmas, espiroquetas, clamidias y rickettsias. Se clasifica en la actualidad de acuerdo con la cinética de muerte bacteriana como co-dependiente. En la bibliografía científica existen trabajos publicados de farmacocinética de oxitetraciclina en distintas especies animales, sin embargo hay escasos trabajos realizados en el cerdo. Dado que es necesario conocer la disposición de un fármaco en la especie animal estudiada para diseñar un adecuado régimen de dosificación, los objetivos del presente trabajo han sido: (i) describir el perfil farmacocinético de la oxitetraciclina tras administración oral única y múltiple en cerdos (Sus scrofa domestica) y (ii) realizar el análisis PK-PD para predecir la eficacia terapeútica del régimen de dosificación...