14,470 research outputs found
Compositional dependence of the strain-free optical band gap in InxGa1 - xN layers
The effect of strain on the compositional and optical properties of a set of epitaxial single layers of
InxGa12xN was studied. Indium content was measured free from the effects of strain by Rutherford
backscattering spectrometry. Accurate knowledge of the In mole fraction, combined with x-ray
diffraction measurements, allows perpendicular strain (e zz) to be evaluated. Optical band gaps were
determined by absorption spectroscopy and corrected for strain. Following this approach, the strain
free dependence of the optical band gap in InxGa12xN alloys was determined for x<0.25. Our
results indicate an ‘‘anomalous,’’ linear, dependence of the energy gap on the In content, at room
temperature: Eg(x)53.39– 3.57x eV. Extension of this behavior to higher concentrations is
discussed on the basis of reported result
Alternativas de controle para redução de grãos ardidos na cultura do milho.
As podridões de espiga e grãos ardidos estão entre as principais doenças da cultura do milho. O presente trabalho teve como objetivo avaliar o efeito da resistência genética e densidade de plantio na incidência de grãos ardidos na cultura do milho. O experimento de resistência genética foi conduzido nas cidades de Indianópolis -MG e Guarda-Mor –MG. O experimento de densidade de plantio foi conduzido na cidade de Sete Lagoas –MG. Realizaram-se identificação e quantificação dos grãos ardidos das amostras de grãos colhidos nos experimentos. Foi realizado o Teste de Patologia de Sementes, através do método do papel de filtro umedecido, para identificação dos fungos associados à ocorrência de grãos ardidos. Foram identificadas cultivares com alto nível de resistência a grãos ardidos. O aumento da densidade de plantio resultou em aumento na incidência de grãos ardidos. De acordo com os resultados obtidos, conclui-se que a resistência genética é uma alternativa viável de controle de fungos que atacam as espigas, e o aumento na densidade de plantio influencia a incidência de grãos ardidos na cultura do milho
The Shape and Scale of Galactic Rotation from Cepheid Kinematics
A catalog of Cepheid variables is used to probe the kinematics of the
Galactic disk. Radial velocities are measured for eight distant Cepheids toward
l = 300; these new Cepheids provide a particularly good constraint on the
distance to the Galactic center, R_0. We model the disk with both an
axisymmetric rotation curve and one with a weak elliptical component, and find
evidence for an ellipticity of 0.043 +/- 0.016 near the Sun. Using these
models, we derive R_0 = 7.66 +/- 0.32 kpc and v_circ = 237 +/- 12 km/s. The
distance to the Galactic center agrees well with recent determinations from the
distribution of RR Lyrae variables, and disfavors most models with large
ellipticities at the solar orbit.Comment: 36 pages, LaTeX, 10 figure
The galactic population of white dwarfs
Original paper can be found at: http://www.iop.org/EJ/conf DOI: 10.1088/1742-6596/172/1/012004 [16th European White Dwarfs Workshop]The contribution of white dwarfs of the different Galactic populations to the stellar content of our Galaxy is only poorly known. Some authors claim a vast population of halo white dwarfs, which would be in accordance with some investigations of the early phases of Galaxy formation claiming a top-heavy initial– mass– function. Here, I present a model of the population of white dwarfs in the Milky Way based on observations of the local white dwarf sample and a standard model of Galactic structure. This model will be used to estimate the space densities of thin disc, thick disc and halo white dwarfs and their contribution to the baryonic mass budget of the Milky Way. One result of this investigation is that white dwarfs of the halo population contribute a large fraction of the Galactic white dwarf number count, but they are not responsible for the lion's share of stellar mass in the Milky Way. Another important result is the substantial contribution of the – often neglected – population of thick disc white dwarfs. Misclassification of thick disc white dwarfs is responsible for overestimates of the halo population in previous investigations.Peer reviewe
Identification of transitional disks in Chamaeleon with Herschel
Transitional disks are circumstellar disks with inner holes that in some
cases are produced by planets and/or substellar companions in these systems.
For this reason, these disks are extremely important for the study of planetary
system formation. The Herschel Space Observatory provides an unique opportunity
for studying the outer regions of protoplanetary disks. In this work we update
previous knowledge on the transitional disks in the Chamaeleon I and II regions
with data from the Herschel Gould Belt Survey. We propose a new method for
transitional disk classification based on the WISE 12 micron-PACS 70 micron
color, together with inspection of the Herschel images. We applied this method
to the population of Class II sources in the Chamaeleon region and studied the
spectral energy distributions of the transitional disks in the sample. We also
built the median spectral energy distribution of Class II objects in these
regions for comparison with transitional disks. The proposed method allows a
clear separation of the known transitional disks from the Class II sources. We
find 6 transitional disks, all previously known, and identify 5 objects
previously thought to be transitional as possibly non-transitional. We find
higher fluxes at the PACS wavelengths in the sample of transitional disks than
those of Class II objects. We show the Herschel 70 micron band to be an
efficient tool for transitional disk identification. The sensitivity and
spatial resolution of Herschel reveals a significant contamination level among
the previously identified transitional disk candidates for the two regions,
which calls for a revision of previous samples of transitional disks in other
regions. The systematic excess found at the PACS bands could be a result of the
mechanism that produces the transitional phase, or an indication of different
evolutionary paths for transitional disks and Class II sources.Comment: Accepted for publication in A&A: 11 March 2013 11 pages, 15 figure
Pollen mother cells of Tradescantia clone 4430 and Tradescantia pallida var. purpurea are equally sensitive to the clastogenic effects of X-rays.
The Tradescantia micronucleus test is a sensitive bioassay for mutagenesis that may be employed both under field and laboratory conditions. This test has been standardized mostly on the basis of the results obtained with clone 4430. However, this clone is not well adapted to tropical weather, frequently showing problems with growth and flowering. In addition, it is attacked by parasites and insects, a fact that limits its use in field studies aiming at the biomonitoring of air pollution. In the city of São Paulo, Tradescantia pallida (Rose) Hunt. var. purpurea Boom is widely distributed as an ornamental plant in gardens and along roadsides and streets, mostly because of its natural resistance and its easy propagation. In this report, we present dose-response curves indicating that the sensitivity of T. pallida and clone 4430 to X-radiation (1, 10, 25 and 50 cGy) is similar. The results confirm our previous suggestion that T. pallida represents a good alternative for in situ mutagenesis testing in tropical regions, especially biomonitoring studies in which the exposure conditions may not be fully controllable
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