The outburst decay of the low magnetic field magnetar SGR 0418+5729

We report on the long-term X-ray monitoring of the outburst decay of the low magnetic field magnetar SGR 0418+5729 using all the available X-ray data obtained with RXTE, Swift, Chandra, and XMM-Newton observations from the discovery of the source in 2009 June up to 2012 August. The timing analysis allowed us to obtain the first measurement of the period derivative of SGR 0418+5729: ˙ P = 4(1) × 10−15 s s−1, significant at a ∼3.5σ confidence level. This leads to a surface dipolar magnetic field of Bdip 6 × 1012 G. This measurement confirms SGR 0418+5729 as the lowest magnetic field magnetar. Following the flux and spectral evolution from the beginning of the outburst up to ∼1200 days, we observe a gradual cooling of the tiny hot spot responsible for the X-ray emission, from a temperature of ∼0.9 to 0.3 keV. Simultaneously, the X-ray flux decreased by about three orders of magnitude: from about 1.4 × 10−11 to 1.2 × 10−14 erg s−1 cm−2. Deep radio, millimeter, optical, and gamma-ray observations did not detect the source counterpart, implying stringent limits on its multi-band emission, as well as constraints on the presence of a fossil disk. By modeling the magneto-thermal secular evolution of SGR 0418+5729, we infer a realistic age of ∼550 kyr, and a dipolar magnetic field at birth of ∼1014 G. The outburst characteristics suggest the presence of a thin twisted bundle with a small heated spot at its base. The bundle untwisted in the first few months following the outburst, while the hot spot decreases in temperature and size. We estimate the outburst rate of low magnetic field magnetars to be about one per year per galaxy, and we briefly discuss the consequences of such a result in several other astrophysical contexts.

Acciones públicas de sensibilización de género: el esfuerzo de la administración regional y local en comunicación publicitaria (1999-2007)

El artículo analiza las iniciativas de comunicación relacionadas con la igualdad de oportunidades entre mujeres y hombres. El objetivo es analizar con enfoque de género las acciones realizadas por parte de las instituciones públicas regionales y locales para sensibilizar y promover la conciliación entre la vida familiar y laboral de seis comunidades autónomas (Andalucía, Cataluña, Comunidad Valenciana, Galicia, Madrid y País Vasco) y de sus capitales, desde 1999 (cuando se aprueba la ley de conciliación) hasta 2007 (se aprueba la ley de igualdad). La información sobre publicidad convencional fue proporcionada por Infoadex. Para la recogida de otro tipo de iniciativas a través de medios menos convencionales se acudió a cuatro fuentes institucionales: 1) Ayuntamientos de las capitales, como fuente estrictamente local, 2) Diputaciones de la capital de la Comunidad Autónoma, como fuente provincial, 3) Direcciones Generales de la Mujer o instituciones análogas como fuente de información a nivel regional o autonómico y, por último, 4) otras concejalías vinculadas al tema de la corresponsabilidad, cuyo radio de acción también es autonómico. Los resultados, aunque con diferencias entre regiones, reflejan carencias en la cobertura de las acciones que llevan a cuestionar la falta de estrategia política en términos de comunicación, pese a la introducción sistemática de estos objetivos en la agenda internacional (ONU y UE) y del gobierno español. En consecuencia, las campañas publicitarias e iniciativas recogidas contribuyen a la visibilización del problema y al empoderamiento, pero no tanto al objetivo de la paridad.

A Computational Method based on Radio Frequency Technologies for the Analysis of Accessibility of Disabled People in Sustainable Cities

The sustainability strategy in urban spaces arises from reflecting on how to achieve a more habitable city and is materialized in a series of sustainable transformations aimed at humanizing different environments so that they can be used and enjoyed by everyone without exception and regardless of their ability. Modern communication technologies allow new opportunities to analyze efficiency in the use of urban spaces from several points of view: adequacy of facilities, usability, and social integration capabilities. The research presented in this paper proposes a method to perform an analysis of movement accessibility in sustainable cities based on radio frequency technologies and the ubiquitous computing possibilities of the new Internet of Things paradigm. The proposal can be deployed in both indoor and outdoor environments to check specific locations of a city. Finally, a case study in a controlled context has been simulated to validate the proposal as a pre-deployment step in urban environments.

Population synthesis of isolated neutron stars with magneto-rotational evolution – II. From radio-pulsars to magnetars

Population synthesis studies constitute a powerful method to reconstruct the birth distribution of periods and magnetic fields of the pulsar population. When this method is applied to populations in different wavelengths, it can break the degeneracy in the inferred properties of initial distributions that arises from single-band studies. In this context, we extend previous works to include X-ray thermal emitting pulsars within the same evolutionary model as radio-pulsars. We find that the cumulative distribution of the number of X-ray pulsars can be well reproduced by several models that, simultaneously, reproduce the characteristics of the radio-pulsar distribution. However, even considering the most favourable magneto-thermal evolution models with fast field decay, lognormal distributions of the initial magnetic field overpredict the number of visible sources with periods longer than 12 s. We then show that the problem can be solved with different distributions of magnetic field, such as a truncated lognormal distribution, or a binormal distribution with two distinct populations. We use the observational lack of isolated neutron stars (NSs) with spin periods P > 12 s to establish an upper limit to the fraction of magnetars born with B > 1015 G (less than 1 per cent). As future detections keep increasing the magnetar and high-B pulsar statistics, our approach can be used to establish a severe constraint on the maximum magnetic field at birth of NSs.