Los depósitos lacustres del Terciario de Bicorp (Valencia)

La Cuenca de Bicorp pertenece al conjunto de cuencas sinorogénicas del Terciario de la província de Valencia. Está emplazada en el sector sur de la zoia de transición entre la cadena  ibérica y las Béticas. La Cuenca de Bicorp es una cuenca continental emplazada sobre un substrato mesozoico formado por materiales triásicos, jurásicos y cretácicos. Sus limites norte y sur son dos fallas normales de orientación ENE-WSW, las cuales actuaron sinsedimentariamente. Los depósitos de la Cuenca de Bicorp tienen un espesor máximo de 450 metros. La base de la serie está formada por materiales de origen aluvial, mientras que el resto lo constituyen facies lacustres. En los depósitos lacustres pueden reconocerse cuatro unidades formadas, desde la base hacia el techo, por: a) margas carbonosas grises, b) calizas laminadas y margas con lignito, c) yesos seleniticos y d) alternancias de calizas y pelitas laminadas bituminosas. De estas unidades la que posee los depósitos de mayor potencia y extensión areal, es la formada por las alternancias de calizas y pelitas bituminosas. Estos son los materiales que caracterizan mejor la serie de la cuenca lacustre de Bicorp. Las alternancias de calizas y pelitas bituminosas están organizadas en secuencias, estrato- y granocrecientes hacia el techo, que se repiten cíclicamente. Cada secuencia está formada por un término superior de calizas y otro inferior de pelitas bituminosas. Las calizas están compuestas, en su mayor parte, por restos esqueléticos de invertebrados acuáticos, y presentan en su techo evidencias de emersión subarea (grietas de desecación, huellas de vertebrados terrestres...). Las pelitas bituminosas se caracterizan por su alto contenido en materia orgánica y por tener una laminación continua milimétrica. Sus características son indicativas de haber sido formadas en un ambiente sin el contenido de oxigeno necesario para permitir la presencia de fauna bentónica en el fondo. En su conjunto, los depósitos de la Cuenca de Bicorp son representativos de un ambiente lacustre salino con unestado permanente de estratificación de sus aguas y con un epilimnion oxigenado y un hipolimnion anóxico

Solvable Lie algebras are not that hypo

We study a type of left-invariant structure on Lie groups, or equivalently on Lie algebras. We introduce obstructions to the existence of a hypo structure, namely the 5-dimensional geometry of hypersurfaces in manifolds with holonomy SU(3). The choice of a splitting g^*=V_1 + V_2, and the vanishing of certain associated cohomology groups, determine a first obstruction. We also construct necessary conditions for the existence of a hypo structure with a fixed almost-contact form. For non-unimodular Lie algebras, we derive an obstruction to the existence of a hypo structure, with no choice involved. We apply these methods to classify solvable Lie algebras that admit a hypo structure.Comment: 21 pages; v2: presentation improved, typos corrected, notational conflicts eliminated. To appear in Transformation Group

The very faint X-ray binary IGR J17062-6143: a truncated disc, no pulsations, and a possible outflow

We present a comprehensive X-ray study of the neutron star low-mass X-ray binary IGR J17062-6143, which has been accreting at low luminosities since its discovery in 2006. Analysing NuSTAR, XMM–Newton, and Swift observations, we investigate the very faint nature of this source through three approaches: modelling the relativistic reflection spectrum to constrain the accretion geometry, performing high-resolution X-ray spectroscopy to search for an outflow, and searching for the recently reported millisecond X-ray pulsations. We find a strongly truncated accretion disc at 77+22−18 gravitational radii (∼164 km) assuming a high inclination, although a low inclination and a disc extending to the neutron star cannot be excluded. The high-resolution spectroscopy reveals evidence for oxygen-rich circumbinary material, possibly resulting from a blueshifted, collisionally ionized outflow. Finally, we do not detect any pulsations. We discuss these results in the broader context of possible explanations for the persistent faint nature of weakly accreting neutron stars. The results are consistent with both an ultra-compact binary orbit and a magnetically truncated accretion flow, although both cannot be unambiguously inferred. We also discuss the nature of the donor star and conclude that it is likely a CO or O–Ne–Mg white dwarf, consistent with recent multiwavelength modelling

Fuzzy intelligence approach for modeling the migration of contaminants ina reservoir affected by AMD pollution

The Sancho Reservoir, located in the Huelva province (SW Spain), is supplied by the Meca River, which receives water contaminated by mining activities in Tharsis. This study focused on determining the relationship that temperature, pH, and electrical conductivity (EC) had with rainfall. The temperature, pH, and EC were simultaneously measured every 30 min by two probes suspended in the Sancho Reservoir. It was anticipated that the use of fuzzy logic and data mining would lead to a model that would show how the contaminant load evolved over space and time. Similar results were obtained for the two locations, except that the parameters had more outliers near the dam due to the greater distance from the contamination source. As expected, higher pH corresponded with lower EC, since, in the absence of chloride, sulphate was the principal anion. The dependency relationship of the variables as well as the cause–effect relationship with the rate of rainfall was more evident in the up-gradient sampling location than near the dam due to the different residence time and the transit time between the two points

The effect of loading direction and Sn alloying on the deformation modes of Zr: An in-situ neutron diffraction study

Deformation modes (slip and twining) in a strongly textured model hcp alloy system (Zr–Sn) have been investigated using in-situ neutron diffraction and deformation along with complementary electron microscopy. Analysis of the evolution of the intergranular strain evolutions and intensity of specific reflections from neutron diffraction show differential influence of Sn on the extent of twinning too, depending on the deformation direction. While Sn displayed very noticeable influence on twin activity when samples were compressed along a direction that predominantly activates prismatic slip, this effect was not seen when samples were compressed along other different directions. These experimental observations were successfully simulated using a CPFE (crystal plasticity finite element) model that incorporates composition sensitive CRSS (critical resolved shear stress) for slip and composition insensitive CRSS activation of twinning. The success of the CPFE model in capturing the experimental observations with respect to twin evolution suggests that the twinning in Zr is chiefly governed by the initial crystallographic texture and the associated intergranular stress state generated during plastic deformation

Los depósitos lacustres del Terciario de Bicorp (Valencia)

La Cuenca de Bicorp pertenece al conjunto de cuencas sinorogénicas del Terciario de la província de Valencia. Está emplazada en el sector sur de la zoia de transición entre la cadena  ibérica y las Béticas. La Cuenca de Bicorp es una cuenca continental emplazada sobre un substrato mesozoico formado por materiales triásicos, jurásicos y cretácicos. Sus limites norte y sur son dos fallas normales de orientación ENE-WSW, las cuales actuaron sinsedimentariamente. Los depósitos de la Cuenca de Bicorp tienen un espesor máximo de 450 metros. La base de la serie está formada por materiales de origen aluvial, mientras que el resto lo constituyen facies lacustres. En los depósitos lacustres pueden reconocerse cuatro unidades formadas, desde la base hacia el techo, por: a) margas carbonosas grises, b) calizas laminadas y margas con lignito, c) yesos seleniticos y d) alternancias de calizas y pelitas laminadas bituminosas. De estas unidades la que posee los depósitos de mayor potencia y extensión areal, es la formada por las alternancias de calizas y pelitas bituminosas. Estos son los materiales que caracterizan mejor la serie de la cuenca lacustre de Bicorp. Las alternancias de calizas y pelitas bituminosas están organizadas en secuencias, estrato- y granocrecientes hacia el techo, que se repiten cíclicamente. Cada secuencia está formada por un término superior de calizas y otro inferior de pelitas bituminosas. Las calizas están compuestas, en su mayor parte, por restos esqueléticos de invertebrados acuáticos, y presentan en su techo evidencias de emersión subarea (grietas de desecación, huellas de vertebrados terrestres...). Las pelitas bituminosas se caracterizan por su alto contenido en materia orgánica y por tener una laminación continua milimétrica. Sus características son indicativas de haber sido formadas en un ambiente sin el contenido de oxigeno necesario para permitir la presencia de fauna bentónica en el fondo. En su conjunto, los depósitos de la Cuenca de Bicorp son representativos de un ambiente lacustre salino con unestado permanente de estratificación de sus aguas y con un epilimnion oxigenado y un hipolimnion anóxico

Automated Morphological Classification of SDSS Red Sequence Galaxies

(abridged) In the last decade, the advent of enormous galaxy surveys has motivated the development of automated morphological classification schemes to deal with large data volumes. Existing automated schemes can successfully distinguish between early and late type galaxies and identify merger candidates, but are inadequate for studying detailed morphologies of red sequence galaxies. To fill this need, we present a new automated classification scheme that focuses on making finer distinctions between early types roughly corresponding to Hubble types E, S0, and Sa. We visually classify a sample of 984 non-starforming SDSS galaxies with apparent sizes >14". We then develop an automated method to closely reproduce the visual classifications, which both provides a check on the visual results and makes it possible to extend morphological analysis to much larger samples. We visually classify the galaxies into three bulge classes (BC) by the shape of the light profile in the outer regions: discs have sharp edges and bulges do not, while some galaxies are intermediate. We separately identify galaxies with features: spiral arms, bars, clumps, rings, and dust. We find general agreement between BC and the bulge fraction B/T measured by the galaxy modeling package GIM2D, but many visual discs have B/T>0.5. Three additional automated parameters -- smoothness, axis ratio, and concentration -- can identify many of these high-B/T discs to yield automated classifications that agree ~70% with the visual classifications (>90% within one BC). Both methods are used to study the bulge vs. disc frequency as a function of four measures of galaxy 'size': luminosity, stellar mass, velocity dispersion, and radius. All size indicators show a fall in disc fraction and a rise in bulge fraction among larger galaxies.Comment: 24 pages, 20 figures, MNRAS accepte

The Seventh Data Release of the Sloan Digital Sky Survey

This paper describes the Seventh Data Release of the Sloan Digital Sky Survey (SDSS), marking the completion of the original goals of the SDSS and the end of the phase known as SDSS-II. It includes 11663 deg^2 of imaging data, with most of the roughly 2000 deg^2 increment over the previous data release lying in regions of low Galactic latitude. The catalog contains five-band photometry for 357 million distinct objects. The survey also includes repeat photometry over 250 deg^2 along the Celestial Equator in the Southern Galactic Cap. A coaddition of these data goes roughly two magnitudes fainter than the main survey. The spectroscopy is now complete over a contiguous area of 7500 deg^2 in the Northern Galactic Cap, closing the gap that was present in previous data releases. There are over 1.6 million spectra in total, including 930,000 galaxies, 120,000 quasars, and 460,000 stars. The data release includes improved stellar photometry at low Galactic latitude. The astrometry has all been recalibrated with the second version of the USNO CCD Astrograph Catalog (UCAC-2), reducing the rms statistical errors at the bright end to 45 milli-arcseconds per coordinate. A systematic error in bright galaxy photometr is less severe than previously reported for the majority of galaxies. Finally, we describe a series of improvements to the spectroscopic reductions, including better flat-fielding and improved wavelength calibration at the blue end, better processing of objects with extremely strong narrow emission lines, and an improved determination of stellar metallicities. (Abridged)Comment: 20 pages, 10 embedded figures. Accepted to ApJS after minor correction