Atmospheric Heating and Wind Acceleration: Results for Cool Evolved Stars based on Proposed Processes

A chromosphere is a universal attribute of stars of spectral type later than ~F5. Evolved (K and M) giants and supergiants (including the zeta Aurigae binaries) show extended and highly turbulent chromospheres, which develop into slow massive winds. The associated continuous mass loss has a significant impact on stellar evolution, and thence on the chemical evolution of galaxies. Yet despite the fundamental importance of those winds in astrophysics, the question of their origin(s) remains unsolved. What sources heat a chromosphere? What is the role of the chromosphere in the formation of stellar winds? This chapter provides a review of the observational requirements and theoretical approaches for modeling chromospheric heating and the acceleration of winds in single cool, evolved stars and in eclipsing binary stars, including physical models that have recently been proposed. It describes the successes that have been achieved so far by invoking acoustic and MHD waves to provide a physical description of plasma heating and wind acceleration, and discusses the challenges that still remain.Comment: 46 pages, 9 figures, 1 table; modified and unedited manuscript; accepted version to appear in: Giants of Eclipse, eds. E. Griffin and T. Ake (Berlin: Springer

The European Solar Telescope

The European Solar Telescope (EST) is a project aimed at studying the magnetic connectivity of the solar atmosphere, from the deep photosphere to the upper chromosphere. Its design combines the knowledge and expertise gathered by the European solar physics community during the construction and operation of state-of-the-art solar telescopes operating in visible and near-infrared wavelengths: the Swedish 1m Solar Telescope, the German Vacuum Tower Telescope and GREGOR, the French Télescope Héliographique pour l'Étude du Magnétisme et des Instabilités Solaires, and the Dutch Open Telescope. With its 4.2 m primary mirror and an open configuration, EST will become the most powerful European ground-based facility to study the Sun in the coming decades in the visible and near-infrared bands. EST uses the most innovative technological advances: the first adaptive secondary mirror ever used in a solar telescope, a complex multi-conjugate adaptive optics with deformable mirrors that form part of the optical design in a natural way, a polarimetrically compensated telescope design that eliminates the complex temporal variation and wavelength dependence of the telescope Mueller matrix, and an instrument suite containing several (etalon-based) tunable imaging spectropolarimeters and several integral field unit spectropolarimeters. This publication summarises some fundamental science questions that can be addressed with the telescope, together with a complete description of its major subsystems

A Mutation in MFSD8 Causes Neuronal Ceroid Lipofuscinosis in Chihuahua Dogs

No abstract available

Superstimulation prior to the ovum pick-up to improve in vitro embryo production in lactating and non-lactating Holstein cows

AbstractThe present study evaluated the efficacy of superstimulation with p-FSH (Folltropin) before the ovum pick-up (OPU) on IVP in lactating and nonlactating Holstein donors. A total of 30 Holstein cows (15 lactating and 15 nonlactating) were blocked by lactation status to one of two groups (control or p-FSH), in a cross-over design. On a random day of the estrous cycle, all cows received an intravaginal progesterone device and 2.0 mg IM of estradiol benzoate (Day 0). Cows in the control group received no further treatment, whereas cows in the p-FSH group received a total dosage of 200 mg of p-FSH on Days 4 and 5 in four decreasing doses 12 hours apart (57, 57, 43, and 43 mg). On Day 7, the progesterone device was removed, and OPU was conducted in both groups (40 hours after the last p-FSH injection in the p-FSH–treated group). There was no difference between groups (P = 0.92) in the numbers of follicles that were aspirated per OPU session (17.2 ± 1.3 vs. 17.1 ± 1.1 in control and p-FSH-treated cows, respectively); however, p-FSH-treated cows had a higher (P < 0.001) percentage of medium-sized follicles (6–10 mm) at the time of the OPU (55.1%; 285/517) than control cows (20.8%; 107/514). Although recovery rate was lower (60.0%, 310/517 vs. 69.8%, 359/514; P = 0.002), p-FSH-treated cows had a higher blastocyst production rate (34.5%, 89/258 vs. 19.8%, 55/278; P < 0.001) and more transferable embryos per OPU session were produced in the p-FSH group (3.0 ± 0.5 vs. 1.8 ± 0.4; P = 0.02). Regardless of treatment, non-lactating cows had a higher blastocyst rate (41.9%, 106/253 vs. 13.4%, 38/283; P = 0.001) and produced more transferable embryos per OPU session (3.5 ± 0.5 vs. 1.3 ± 0.3; P = 0.003) than lactating cows. Thus, superstimulation of Holstein donors with p-FSH before OPU increased the efficiency of IVP. In addition, non-lactating donors had higher percentage of in vitro blastocyst development and produced more embryos per OPU session than lactating cows

Herpes Zoster oftálmico e posterior acidente vascular cerebral: relato de caso

Um caso de acidente vascular cerebral (AVC) 14 semanas após a instalação de herpes zoster oftálmico (HZO) é apresentado. A tomografia computadorizada craniana documentou comprometimento em território de artéria cerebral média ipsilateral ao HZO. O diagnóstico de probabilidade é o de arterite por herpes zoster com posterior trombose. Os autores reviram a literatura e enfatizam o longo intervalo entre o HZO e a instalação da hemiplegia. Citam as novas drogas antivirais que tornam esta causa de AVC potencialmente passível de ser prevenida

H-ABC syndrome and DYT4: Variable expressivity or pleiotropy of TUBB4 mutations?

Recently, mutations in the TUBB4A gene have been found to underlie hypomyelination with atrophy of the basal ganglia and cerebellum (H-ABC) syndrome, a rare neurodegenerative disorder of infancy and childhood. TUBB4A mutations also have been described as causative of DYT4 (&quot;hereditary whispering dysphonia&quot;). However, in DYT4, brain imaging has been reported to be normal and, therefore, H-ABC syndrome and DYT4 have been construed to be different disorders, despite some phenotypic overlap. Hence, the question of whether these disorders reflect variable expressivity or pleiotropy of TUBB4A mutations has been raised. We report four unrelated patients with imaging findings either partially or totally consistent with H-ABC syndrome, who were found to have TUBB4A mutations. All four subjects had a relatively homogenous phenotype characterized by severe generalized dystonia with superimposed pyramidal and cerebellar signs, and also bulbar involvement leading to complete aphonia and swallowing difficulties, even though one of the cases had an intermediate phenotype between H-ABC syndrome and DYT4. Genetic analysis of the TUBB4A gene showed one previously described and two novel mutations (c.941C&gt;T; p.Ala314Val and c.900G&gt;T; p.Met300Ile) in the exon 4 of the gene. While expanding the genetic spectrum of H-ABC syndrome, we confirm its radiological heterogeneity and demonstrate that phenotypic overlap with DYT4. Moreover, reappraisal of previously reported cases would also argue against pleiotropy of TUBB4A mutations. We therefore suggest that H-ABC and DYT4 belong to a continuous phenotypic spectrum associated with TUBB4A mutations. © 2014 International Parkinson and Movement Disorder Society