Memòries manuscrites de la Reial Acadèmia de Medicina de Catalunya

Aquesta publicació és un primer pas de cara a recuperar les memòries guardades a la Reial Acadèmia de Medicina de Catalunya i que suposen un fons molt útil per a conèixer la realitat de la pràctica mèdica durant la primera meitat del segle XIX. Aquí es proporciona un catàleg que recull les referències de les 339 memòries manuscrites que es guarden a l'acadèmia corresponents a aquest període.

Les Topografies mèdiques de la Reial Acadèmia de Medicina de Catalunya

En aquesta publicació el doctor Vallribera enumera part del fons no catalogat de la Reial Acadèmia de Medicina de Catalunya, en concret 145 memòries trameses a l¿Acadèmia per tal d¿optar als premis de Topografies Mèdiques. L¿autor n¿enumera les característiques i afegeix una valoració personal.El valor dels treballs recollits rau en la diversitat d¿enfocaments dintre de la temàtica sanitària i en el seu considerable interès sociològic i per a la petita història local, doncs força d¿aquestes memòries es refereixen a poblacions catalanes però també a algunes espanyoles i fins i tot de les filipines.

Catalogo de la flora bentonica marina de las Islas Baleares II: Phaeophyceae, Chlorophyceae

Este catálogo incluye 79 Feofíceas y 68 Clorofíceas que pertenecen a la flora bentónica balear. La flora bentónica marina de las Baleares, a causa de la elevada temperatura del agua, presenta cierta tropicalidad, carácter que queda reflejado en el elevado valor del índice R/P.

Catàleg florístic del Moianès i àrees properes. Primera versió

La següent llista inclou tots els tàxons observats per l'autor en el territori del Moianès i àrees properes (en vermell en el mapa adjunt al final del text) fins al moment, tan espontanis com subespontanis o naturalitzats.Alguns grups complexos resten encara en procés de revisió (gèneres Asplenium, Festuca, Rubus, Hieracium p.p., Ophrys¿). També s'han mantingut espècies àmplies (a nivell de grup) en els casos en que encara falta una revisió definitiva de quins tàxons a nivell infraespecífic són presents al territori. Cal també fer esment del caràcter no exhaustiu de les espècies al·lòctones recollides, especialment de les considerades subespontànies.Pel que fa a la nomenclatura i taxonomia s'ha seguit en la majoaria dels casos la Flora Manual dels Països Catalans (Bolòs et al., 2005). L'índex de raresa utilitzat segueix la següent escala: C: comú; F: freqüent; R: rar; RR: molt rar.

Optical spectroscopy of microquasar candidates at low Galactic latitudes

We report optical spectroscopic observations of a sample of 6 low-galactic latitude microquasar candidates selected by cross-identification of X-ray and radio point source catalogs for |b|<5 degrees. Two objects resulted to be of clear extragalactic origin, as an obvious cosmologic redshift has been measured from their emission lines. For the rest, none exhibits a clear stellar-like spectrum as would be expected for genuine Galactic microquasars. Their featureless spectra are consistent with being extragalactic in origin although two of them could be also highly reddened stars. The apparent non-confirmation of our candidates suggests that the population of persistent microquasar systems in the Galaxy is more rare than previously believed. If none of them is galactic, the upper limit to the space density of new Cygnus X-3-like microquasars within 15 kpc would be 1.1\times10^{-12} per cubic pc. A similar upper limit for new LS 5039-like systems within 4 kpc is estimated to be 5.6\times10^{-11} per cubic pc.

EVN+MERLIN observations of microquasar candidates at low galactic latitudes

In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a long-term project focused on the search for new objects of this type. They performed a cross-identification between X-ray and radio catalogs under very restrictive selection criteria for sources with |b|<5 degrees, and obtained a sample of 13 radio-emitting X-ray sources. Follow-up observations of 6 of these sources with the VLA provided accurate coordinates, which were used to discover optical counterparts for all of them. We have observed these six sources with the EVN and MERLIN at 5 GHz. Five of the six objects have been detected and imaged, presenting different morphologies: one source has a two-sided jet, three sources have one-sided jets, and one source is compact. With all the presently available information, we conclude that two of the sources are promising microquasar candidates in our Galaxy.

L’experiència del CRAI de la UB en la migració consorciada a Millennium

Aquest article pretén reflectir l'experiència viscuda a la Universitat de Barcelona (UB) en el procés viscut fa poc de canvi de sistema de Catàleg Col·lectiu de les Universitats de Catalunya (CCUC) i dels catàlegs de les institucions del Consorci de Biblioteques Universitàries de Catalunya (CBUC). Es recullen les principals actuacions i fites tècniques i organitzatives que ha assolit l'equip responsable de la implementació en les diferents fases del projecte, des d'un punt de vista professional però, sobretot, des del punt de vista personal d'implicació, de repte, de satisfacció i d'esforç. Es conclou destacant, d'una banda, la rellevància del treball en equip com a factor d'èxit en el desenvolupament d'un projecte complexi, de l'altra, la necessitat d'una reflexió global sobre els processos i fluxos de treball, per tal d'explotar al màxim les possibilitats d'un sistema de gestió integral i aconseguir el màxim d'eficiència.

The Coordinated Radio and Infrared Survey for High-mass Star Formation. II. Source Catalog

The CORNISH project is the highest resolution radio continuum survey of the Galactic plane to date. It is the 5 GHz radio continuum part of a series of multi-wavelength surveys that focus on the northern GLIMPSE region (10° < l < 65°), observed by the Spitzer satellite in the mid-infrared. Observations with the Very Large Array in B and BnA configurations have yielded a 1.''5 resolution Stokes I map with a root mean square noise level better than 0.4 mJy beam 1. Here we describe the data-processing methods and data characteristics, and present a new, uniform catalog of compact radio emission. This includes an implementation of automatic deconvolution that provides much more reliable imaging than standard CLEANing. A rigorous investigation of the noise characteristics and reliability of source detection has been carried out. We show that the survey is optimized to detect emission on size scales up to 14'' and for unresolved sources the catalog is more than 90% complete at a flux density of 3.9 mJy. We have detected 3062 sources above a 7σ detection limit and present their ensemble properties. The catalog is highly reliable away from regions containing poorly sampled extended emission, which comprise less than 2% of the survey area. Imaging problems have been mitigated by down-weighting the shortest spacings and potential artifacts flagged via a rigorous manual inspection with reference to the Spitzer infrared data. We present images of the most common source types found: H II regions, planetary nebulae, and radio galaxies. The CORNISH data and catalog are available online at http://cornish.leeds.ac.uk.

Scientific journals in Brazil and Spain: Alternative publishing models

This paper describes high-quality journals in Brazil and Spain, with an emphasis on the distribution models used. It presents the general characteristics (age, type of publisher, and theme) and analyzes the distribution model by studying the type of format (print or digital), the type of access (open access or subscription), and the technology platform used. The 549 journals analyzed (249 in Brazil and 300 in Spain) are included in the 2011 Web of Science (WoS) and Scopus databases. Data on each journal were collected directly from their websites between March and October 2012. Brazil has a fully open access distribution model (97%) in which few journals require payment by authors thanks to cultural, financial, operational, and technological support provided by public agencies. In Spain, open access journals account for 55% of the total and have also received support from public agencies, although to a lesser extent. These results show that there are systems support of open access in scientific journals other than the"author pays" model advocated by the Finch report for the United Kingdom.