Abstract The environment of the high-redshift ( z = 1.408), powerful radio-loud galaxy 3C 297 has several distinctive features a cluster. Among them, characteristic halo hot gas revealed by Chandra X-ray observations. In addition, radio map obtained with Very Large Array shows bright hotspot in northwestern direction, created interaction active galactic nucleus (AGN) jet arising from its enviro...

Irritable bowel syndrome (IBS) is one of the most common functional gastrointestinal disorders in adults, children, and adolescents. This paper reviews etiology pathogenesis IBS, particularly its subtypes, postinfectious associated with a prior acute intestinal infection. The authors discuss risk factors, diagnosis, treatment for IBS describe diagnostic search therapeutic algorithm child. Treat...

Background: Iguratimod (IGU) has demonstrated efficacy and safety for active rheumatoid arthritis (RA) patients in double-blind clinical trials China Japan as a new disease-modifying anti-rheumatic drug (DMARD). There are no studies evaluating the radiographic progression of structural joint damage IGU treatment RA using mTSS primary endpoint. Objectives: Our study was to evaluate monotherapy c...

INTRODUCTION................................................................................... 281 I. ECONOMIC CONCERNS ........................................................... 283 II. TECHNICAL CONCERNS: A CABLELABS CASE STUDY......... 287 A. DOCSIS .............................................................................. 288 B. PacketCable................................................

Quisiera expresar mi profunda gratitud por el gran honor que me han con-cedido de presentar esta obra recoge Homilías Mons. Moreno du-rante año 2006, textos fueron cuidadosamente seleccionados, orde-nados, corregidos y subrayados Monseñor en sus últimos años vividos la Casa del Clero Concepción.

Abstract MWC 297 is a young, early-type star driving an ionized outflow and surrounded by warm, entrained dust. Previous analyses of near- mid-IR interferometric images suggest that the emission at these wavelengths arises from compact accretion disk with moderate ( i < 40°) inclination. We have obtained 5–40 μ m FORCAST on SOFIA, as well near-infrared spectra acquired SpeX IRTF radio data V...