Trabajos de seguimiento de la lapa ferruginosa Patella ferruginea Gmelin, 1791 en Andalucía en el marco de la Estrategia Nacional de Conservación de la especie

El gasterópodo marino Patella ferruginea se encuentra incluido en los Catálogos Español y Andaluz de Especies Amenazadas en la categoría “En peligro de extinción”. En 2008 fue aprobada la Estrategia de Conservación Nacional de la especie que establece la realización de un seguimiento de la población cada cuatro años. En Andalucía se ha realizado en 2010 el seguimiento de la especie empleando dos tipos de metodología: los “Controles de crecimiento”, mediante marcaje de ejemplares, y los “Censos exhaustivos” en “Tramos” de costa, para intentar detectar todos los individuos presentes. En el censo de 2010 se han muestreado unos 21 km de costa en 34 localidades, un 5% del litoral andaluz con presencia de la especie, lo que constituye un esfuerzo considerable, pero asumible para el control periódico de la misma. La densidad media detectada es muy baja, de 0,048 ind./m. El mayor número de individuos se encuentra en Cádiz y la población mejor estructurada en la isla de Alborán. Se estima que el tamaño actual de la población en Andalucía ronda los 1.800 ejemplares, lo que constituye un aumento con respecto a inventarios anteriores. Sin embargo, el contingente es muy reducido para garantizar la supervivencia de la especie. La categoría de protección propuesta por el Libro Rojo de los Invertebrados de Andalucía, “En peligro crítico” (MORENO y ARROYO, 2008), debe considerarse, por lo tanto, la más adecuada para la lapa ferruginosa siguiendo los criterios de valoración de la UICN (2001).

Plastisol foaming process. Decomposition of the foaming agent, polymer behavior in the corresponding temperature range and resulting foam properties

The decomposition of azodicarbonamide, used as foaming agent in PVC—plasticizer (1/1) plastisols was studied by DSC. Nineteen different plasticizers, all belonging to the ester family, two being polymeric (polyadipates), were compared. The temperature of maximum decomposition rate (in anisothermal regime at 5 K min−1 scanning rate), ranges between 434 and 452 K. The heat of decomposition ranges between 8.7 and 12.5 J g−1. Some trends of variation of these parameters appear significant and are discussed in terms of solvent (matrix) and viscosity effects on the decomposition reactions. The shear modulus at 1 Hz frequency was determined at the temperature of maximum rate of foaming agent decomposition, and differs significantly from a sample to another. The foam density was determined at ambient temperature and the volume fraction of bubbles was used as criterion to judge the efficiency of the foaming process. The results reveal the existence of an optimal shear modulus of the order of 2 kPa that corresponds roughly to plasticizer molar masses of the order of 450 ± 50 g mol−1. Heavier plasticizers, especially polymeric ones are too difficult to deform. Lighter plasticizers such as diethyl phthalate (DEP) deform too easily and presumably facilitate bubble collapse.

On the formation and evolution of the first Be star in a black hole binary MWC 656

We find that the formation of MWC 656 (the first Be binary containing a black hole) involves a common envelope phase and a supernova explosion. This result supports the idea that a rapidly rotating Be star can emerge out of a common envelope phase, which is very intriguing because this evolutionary stage is thought to be too fast to lead to significant accretion and spin up of the B star. We predict ∼10–100 of B-BH binaries to currently reside in the Galactic disc, among which around 1/3 contain a Be star, but there is only a small chance to observe a system with parameters resembling MWC 656. If MWC 656 is representative of intrinsic Galactic Be-BH binary population, it may indicate that standard evolutionary theory needs to be revised. This would pose another evolutionary problem in understanding black hole (BH) binaries, with BH X-ray novae formation issue being the prime example. Future evolution of MWC 656 with an ∼5 M⊙ BH and with an ∼13 M⊙ main-sequence companion on an ∼60 d orbit may lead to the formation of a coalescing BH–NS (neutron star) system. The estimated Advanced LIGO/Virgo detection rate of such systems is up to ∼0.2 yr−1. This empirical estimate is a lower limit as it is obtained with only one particular evolutionary scenario, the MWC 656 binary. This is only a third such estimate available (after Cyg X-1 and Cyg X-3), and it lends additional support to the existence of so far undetected BH–NS binaries.