Comments On “the Organization Of Pharmaceutical Services By ‘health Region’ In Brazil’s Unified Health System”

This study aimed to describe and characterize the pharmaceutical services provided in Brazil’s Unified Health System (SUS) from the point of view of the healthcare networks that are organized by region in the QualiSUS-Rede Project. This was a cross-sectional study, with data collected from December 2013 to July 2015, in public health establishments that carried out delivery or warehousing of medications (n = 4,938), in 465 municipalites, and the Federal District, in 43‘Health Regions’. The results show the existence of at least one management service supporting the health network, and warehousing of medications in all the regions (> 90%). It also showed the availability of at least one healthcare service, in healthcare locations, by pharmaceutical professionals is irregular between the Regions, being highest in the Southeastern Region (74.3%), and lowest in the Northeastern Region (43.3%). The results underpine the need for effective structuring of pharmaceutical assistance in the SUS networks, overcoming the current restrictive vision of its activities, which gives value almost exclusively to the logistical component of support to the network, to the detriment of the clinical component. It is also important to expand, and improve the quality of, the population’s access to medical drugs, and improve the quality of the healthcare offered to users of the system. © 2017, Associacao Brasileira de Pos - Graduacao em Saude Coletiva. All rights reserved.2241181119

Modelling spectral and timing properties of accreting black holes: the hybrid hot flow paradigm

The general picture that emerged by the end of 1990s from a large set of optical and X-ray, spectral and timing data was that the X-rays are produced in the innermost hot part of the accretion flow, while the optical/infrared (OIR) emission is mainly produced by the irradiated outer thin accretion disc. Recent multiwavelength observations of Galactic black hole transients show that the situation is not so simple. Fast variability in the OIR band, OIR excesses above the thermal emission and a complicated interplay between the X-ray and the OIR light curves imply that the OIR emitting region is much more compact. One of the popular hypotheses is that the jet contributes to the OIR emission and even is responsible for the bulk of the X-rays. However, this scenario is largely ad hoc and is in contradiction with many previously established facts. Alternatively, the hot accretion flow, known to be consistent with the X-ray spectral and timing data, is also a viable candidate to produce the OIR radiation. The hot-flow scenario naturally explains the power-law like OIR spectra, fast OIR variability and its complex relation to the X-rays if the hot flow contains non-thermal electrons (even in energetically negligible quantities), which are required by the presence of the MeV tail in Cyg X-1. The presence of non-thermal electrons also lowers the equilibrium electron temperature in the hot flow model to <100 keV, making it more consistent with observations. Here we argue that any viable model should simultaneously explain a large set of spectral and timing data and show that the hybrid (thermal/non-thermal) hot flow model satisfies most of the constraints.Comment: 26 pages, 13 figures. To be published in the Space Science Reviews and as hard cover in the Space Sciences Series of ISSI - The Physics of Accretion on to Black Holes (Springer Publisher