La coleccion de Centrosema de CIAT: Datos de pasaporte basicos y distribucion geografica del germoplasma en la coleccion de CIAT

Se presentan los datos de pasaporte basicos de la coleccion de Centrosema del CIAT: no. de acceso, fuente, institucion colaboradora, origen, fecha de coleccion y registro, y mapas de la distribucion geografica de las 29 especies que conforman la coleccion. (CIAT

Catalogo de germoplasma de especies forrajeras tropicales

Se presenta un catalogo, compuesto por 3 tomos, con datos de pasaporte basicos de las accesiones de plantas forrajeras del CIAT. El tomo 1 incluye la guia secuencial y las gramineas estan ordenadas alfabeticamente por generos, mientras los tomos 2 y 3 comprenden los generos de leguminosas, de A-G y de H-Z, resp. El catalogo proporciona algunos datos como: no. de acceso, genero/especie, fuente (donacion, recoleccion colaborativa o recoleccion de CIAT), institucion colaboradora, origen, fechas de recoleccion y registro de la accesion. Se indica que algunas accesiones han pasado por una fase de multiplicacion inicial de semillas por parte del Programa de Pastos Tropicales y/o la Unidad de Recursos Geneticos del CIAT, quienes pueden proporcionar pequenas cantidades de semillas para propositos de investigacion. (CIAT

A Systematic Review of Patient- and Family-Level Inhaled Corticosteroid Adherence Interventions in Black/African Americans

Background: Inhaled corticosteroid (ICS) adherence rates are suboptimal among adult black/African Americans. Comprehensive studies characterizing the effectiveness and the methodological approaches to the development of interventions to improve ICS adherence in adult black/African Americans have not been performed. Objectives: Conduct a systematic review of patient/family-level interventions to improve ICS adherence in adult black/African Americans. Methods: We searched MEDLINE, EMBASE, Web of Science, and CINAHL from inception to August 2017 for English-language US studies enrolling at least 30% black/African Americans comparing patient/family-level ICS adherence interventions with any comparator. Two investigators independently selected, extracted data from, and rated risk of bias. We collected information on intervention characteristics and outcomes, and assessed whether studies were informed by behavior theory, stakeholder engagement, or both. Results: Among 1661 abstracts identified, we reviewed 230 full-text articles and identified 4 randomized controlled trials (RCTs) and 1 quasi-experimental (pre-post design) study meeting criteria. Study participants (N range, 17-333) varied in mean age (22-47 years), proportion black/African Americans studied (71%-93%), and sex (69%-82% females). RCTs evaluated problem-solving classes, self-efficacy training, technology-based motivational interviewing program, and the use of patient advocates. The RCT testing self-efficacy training was the only intervention informed by both behavior theory and stakeholder engagement. All 4 RCTs compared interventions with active control and rated as medium risk of bias. No RCTs found a statistically significant improvement in adherence. Conclusions: Few studies assessing asthma adherence interventions focused on adult black/African-American populations. No RCTs demonstrated improved ICS adherence in participants. Future studies that are informed by behavior change theory and stakeholder engagement are needed

Magnetic Field Amplification in Galaxy Clusters and its Simulation

We review the present theoretical and numerical understanding of magnetic field amplification in cosmic large-scale structure, on length scales of galaxy clusters and beyond. Structure formation drives compression and turbulence, which amplify tiny magnetic seed fields to the microGauss values that are observed in the intracluster medium. This process is intimately connected to the properties of turbulence and the microphysics of the intra-cluster medium. Additional roles are played by merger induced shocks that sweep through the intra-cluster medium and motions induced by sloshing cool cores. The accurate simulation of magnetic field amplification in clusters still poses a serious challenge for simulations of cosmological structure formation. We review the current literature on cosmological simulations that include magnetic fields and outline theoretical as well as numerical challenges.Comment: 60 pages, 19 Figure

Horizontal Branch Stars: The Interplay between Observations and Theory, and Insights into the Formation of the Galaxy

We review HB stars in a broad astrophysical context, including both variable and non-variable stars. A reassessment of the Oosterhoff dichotomy is presented, which provides unprecedented detail regarding its origin and systematics. We show that the Oosterhoff dichotomy and the distribution of globular clusters (GCs) in the HB morphology-metallicity plane both exclude, with high statistical significance, the possibility that the Galactic halo may have formed from the accretion of dwarf galaxies resembling present-day Milky Way satellites such as Fornax, Sagittarius, and the LMC. A rediscussion of the second-parameter problem is presented. A technique is proposed to estimate the HB types of extragalactic GCs on the basis of integrated far-UV photometry. The relationship between the absolute V magnitude of the HB at the RR Lyrae level and metallicity, as obtained on the basis of trigonometric parallax measurements for the star RR Lyrae, is also revisited, giving a distance modulus to the LMC of (m-M)_0 = 18.44+/-0.11. RR Lyrae period change rates are studied. Finally, the conductive opacities used in evolutionary calculations of low-mass stars are investigated. [ABRIDGED]Comment: 56 pages, 22 figures. Invited review, to appear in Astrophysics and Space Scienc

A Galaxy-scale Fountain of Cold Molecular Gas Pumped by a Black Hole

We present Atacama Large Millimeter/submillimeter Array and Multi-Unit Spectroscopic Explorer observations of the brightest cluster galaxy in Abell 2597, a nearby (z = 0.0821) cool core cluster of galaxies. The data map the kinematics of a three billion solar mass filamentary nebula that spans the innermost 30 kpc of the galaxy's core. Its warm ionized and cold molecular components are both cospatial and comoving, consistent with the hypothesis that the optical nebula traces the warm envelopes of many cold molecular clouds that drift in the velocity field of the hot X-ray atmosphere. The clouds are not in dynamical equilibrium, and instead show evidence for inflow toward the central supermassive black hole, outflow along the jets it launches, and uplift by the buoyant hot bubbles those jets inflate. The entire scenario is therefore consistent with a galaxy-spanning "fountain," wherein cold gas clouds drain into the black hole accretion reservoir, powering jets and bubbles that uplift a cooling plume of low-entropy multiphase gas, which may stimulate additional cooling and accretion as part of a self-regulating feedback loop. All velocities are below the escape speed from the galaxy, and so these clouds should rain back toward the galaxy center from which they came, keeping the fountain long lived. The data are consistent with major predictions of chaotic cold accretion, precipitation, and stimulated feedback models, and may trace processes fundamental to galaxy evolution at effectively all mass scales

Measurement of the Bottom-Strange Meson Mixing Phase in the Full CDF Data Set

We report a measurement of the bottom-strange meson mixing phase \beta_s using the time evolution of B0_s -> J/\psi (->\mu+\mu-) \phi (-> K+ K-) decays in which the quark-flavor content of the bottom-strange meson is identified at production. This measurement uses the full data set of proton-antiproton collisions at sqrt(s)= 1.96 TeV collected by the Collider Detector experiment at the Fermilab Tevatron, corresponding to 9.6 fb-1 of integrated luminosity. We report confidence regions in the two-dimensional space of \beta_s and the B0_s decay-width difference \Delta\Gamma_s, and measure \beta_s in [-\pi/2, -1.51] U [-0.06, 0.30] U [1.26, \pi/2] at the 68% confidence level, in agreement with the standard model expectation. Assuming the standard model value of \beta_s, we also determine \Delta\Gamma_s = 0.068 +- 0.026 (stat) +- 0.009 (syst) ps-1 and the mean B0_s lifetime, \tau_s = 1.528 +- 0.019 (stat) +- 0.009 (syst) ps, which are consistent and competitive with determinations by other experiments.Comment: 8 pages, 2 figures, Phys. Rev. Lett 109, 171802 (2012