1,199 research outputs found
High Spectral and Spatial Resolution Observations of the PDR Emission in the NGC2023 Reflection Nebula with SOFIA and APEX
We have mapped the NGC 2023 reflection nebula in [CII] and CO(11--10) with
the heterodyne receiver GREAT on SOFIA and obtained slightly smaller maps in
13CO(3--2), CO(3--2), CO(4--3), CO(6--5), and CO(7--6) with APEX in Chile. We
use these data to probe the morphology, kinematics, and physical conditions of
the C II region, which is ionized by FUV radiation from the B2 star HD37903.
The [CII] emission traces an ellipsoidal shell-like region at a position angle
of ~ -50 deg, and is surrounded by a hot molecular shell. In the southeast,
where the C II region expands into a dense, clumpy molecular cloud ridge, we
see narrow and strong line emission from high-J CO lines, which comes from a
thin, hot molecular shell surrounding the [CII] emission. The [CII] lines are
broader and show photo evaporating gas flowing into the C II region. Based on
the strength of the [13CII] F=2--1 line, the [CII] line appears to be somewhat
optically thick over most of the nebula with an optical depth of a few. We
model the physical conditions of the surrounding molecular cloud and the PDR
emission using both RADEX and simple PDR models. The temperature of the CO
emitting PDR shell is ~ 90 -- 120 K, with densities of 10^5 -- 10^6 cm^-3, as
deduced from RADEX modeling. Our PDR modeling indicates that the PDR layer
where [CII] emission dominates has somewhat lower densities, 10^4 to a few
times 10^5 cm^-3Comment: Accepted by A&
Habitat Use, Phenology, And Gregariousness Of The Neotropical Psocopteran Cerastipsocus Sivorii (psocoptera: Psocidae)
A field account of the behavior and ecology of the gregarious and corticolous psocopteran Cerastipsocus sivorii is presented. The study was conducted from February to November 2003 on the campus of the Universidade Estadual de Campinas, state of São Paulo, southeastern Brazil. There was a strong positive correlation between the relative abundance of host tree species and their respective frequency of occupation by C. sivorii, suggesting that trees were used according to their availability in the study site. The phenology of C. sivorii is seasonal, with nymphs peaking in May and October, and teneral adults peaking in February, June, and October. The factors determining the variation in population density in psocopterans are poorly understood, but our data show that climatic variables, such as rainfall and temperature do not influence the phenology of C. sivorii. The individuals of C. sivorii remain together through the entire nymphal phase, resting, moving on the tree surface (mainly on bark, but occasionally on leaf petioles) and grazing in groups. Teneral adults within an aggregation usually dispersed a few days after molting. Nearly 50% of the aggregations had up to 90 individuals, but large groups presenting 240 individuals or more were also frequent, comprising 10% of all aggregations found in the field. When a moving aggregation encountered another one, they occasionally either interchanged individuals or merged into a single large group. More rarely, large aggregations divided into two groups. We suggest that gregariousness in C. sivorii is a behavioral strategy that confers protection against predation and reduces body water loss.493197214Baz, A., Observations on the biology and ecology of Psocoptera found in different kinds of leaf litter in East-Central Spain (1991) Pedobiologia, 35, pp. 89-100Baz, A., Phenology and crypsis as possible determinants of habitat selection in populations of Hemineura bigoti from central Spain (Psocoptera: Elipsocidae) (1992) Entomologia Generalis, 17, pp. 293-298Baz, A., Diversidad y abundancia de los psocópteros frondícolas y corticícolas en el sistema Ibérico Meridional (España Central) (1995) Annales de la Societé Entomologique de France, 31, pp. 71-83Broadhead, E., Psocid fauna of larch trees in Northern England - an ecological study of mixed species population exploiting a common resource (1958) Journal of Animal Ecology, 27, pp. 217-263Broadhead, E., Wapshere, A.J., Mesopsocus populations on larch in England -the distribution and dynamics of two closely-related coexisting species of Psocoptera sharing the same food resource (1966) Ecological Monographs, 36, pp. 326-388Chivers, D.P., Kiesecker, J.M., Anderson, M.T., Wildy, E.L., Blaustein, A.R., Avoidance response of a terrestrial salamander (Ambystoma macrodactylum) to chemical alarm cues (1996) Journal of Chemical Ecology, 22, pp. 1709-1716Daly, H.V., Doyen, J.T., Purcell, A.H., (1998) Introduction to Insect Biology and Diversity, , 2nd ed. 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Las palabras de Max: un cuento moral
Requena, G.; Fernández Requena, A. (1978). Las palabras de Max: un cuento moral. La mirada. (2):26-28. http://hdl.handle.net/10251/41559.Importación Masiva2628
The largest oxigen bearing organic molecule repository
We present the first detection of complex aldehydes and isomers in three
typical molecular clouds located within 200pc of the center of our Galaxy.
We find very large abundances of these complex organic molecules (COMs) in
the central molecular zone (CMZ), which we attribute to the ejection of COMs
from grain mantles by shocks. The relative abundances of the different COMs
with respect to that of CH3OH are strikingly similar for the three sources,
located in very different environments in the CMZ. The similar relative
abundances point toward a unique grain mantle composition in the CMZ. Studying
the Galactic center clouds and objects in the Galactic disk having large
abundances of COMs, we find that more saturated molecules are more abundant
than the non-saturated ones. We also find differences between the relative
abundance between COMs in the CMZ and the Galactic disk, suggesting different
chemical histories of the grain mantles between the two regions in the Galaxy
for the complex aldehydes. Different possibilities for the grain chemistry on
the icy mantles in the GC clouds are briefly discussed. Cosmic rays can play an
important role in the grain chemistry. With these new detections, the molecular
clouds in the Galactic center appear to be one of the best laboratories for
studying the formation of COMs in the Galaxy.Comment: 20 pages, 4 figures, accepted in Ap
Effect of solution heat treatment on the internal architecture and compressive strength of an AlMg4.7Si8 alloy
The evolution of the microstructure of an AlMg4.7Si8 alloy is investigated by scanning electron microscopy and ex situ synchrotron tomography in as-cast condition and subsequent solution treatments for 1 h and 25 h at 540 °C, respectively. The eutectic Mg2Si phase, which presents a highly interconnected structure in the as-cast condition, undergoes significant morphological changes during the solution heat treatment. Statistical analyses of the particle distribution, the sphericity, the mean curvatures and Gaussian curvatures describe the disintegration of the interconnected seaweed-like structure followed by the rounding of the disintegrated fractions of the eutectic branches quantitatively. The ternary eutectic Si resulting from the Si-surplus to the stoichiometric Mg2Si ratio of the alloy undergoes similar changes. The morphological evolution during solution heat treatment is correlated with results of elevated temperature compression tests at 300 °C. The elevated temperature compressive strength is more sensitive to the degree of interconnectivity of the three dimensional Mg2Si network than to the shape of the individual particles. © 2013 Elsevier B.V. All rights reserved
Relato y autor: (con Providence de Resanais como campo de aplicación)
Requena, JG. (1978). Relato y autor: (con Providence de Resanais como campo de aplicación). La mirada. (2):58-64. http://hdl.handle.net/10251/41567.Importación Masiva5864
Sub-micrometre holotomographic characterisation of the effects of solution heat treatment on an AlMg7.3Si3.5 alloy
A strip cast AlMg7.3Si3.5 alloy is investigated by sub-micrometre holotomographic analysis achieving a voxel size of (60 nm)(3) by cone beam magnification of the focused synchrotron beam using Kirkpatrick-Baez mirrors. The three-dimensional microstructure of the same specimen volume in the as-cast state is compared with that after exposure to 540 degrees C for 30 min resolving microstructural features down to 180 nm. The three-dimensional analysis of the architecture of the eutectic Mg2Si and the Fe-aluminides reveals how the as-cast microstructure changes during the solution treatment. The alloy in the as-cast condition contains a highly interconnected seaweed-like Mg2Si eutectic. The level of three-dimensional interconnectivity of the Mg2Si eutectic phase decreases by only partial disintegration during the heat treatment correcting the two-dimensional metallographic impression of isolated round particles. Statistical analyses of the particle distribution, sphericity, mean curvatures and Gaussian curvatures describe quantitatively the architectural changes of the Mg2Si phase. This explains the decrease of the high temperature strength of the alloy by the solution treatment tested in hot compression. (C) 2012 Elsevier B.V. All rights reserved
Burguesía y aparato cinematográfico
Requena, JG. (1978). Burguesía y aparato cinematográfico. La mirada. (1):13-21. http://hdl.handle.net/10251/41546.Importación Masiva1321
Elementos para el análisis de un aparato ideológico
Requena, JG. (1978). Elementos para el análisis de un aparato ideológico. La mirada. (4):41-45. http://hdl.handle.net/10251/41588.Importación Masiva4145
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