1,457 research outputs found
Metodología de investigación de los yacimientos de pizarras para cubiertas
[Resumen] Se exponen .las bases metodológicas autores aplican a la investigación y de yacimientos de pizarras para cubiertas, tanto de su propia experiencia como de bibliografía disponible sobre el tema. Los factores que controlan la calidad de los yacimientos de dicha materia prima son de tres tipos: Litoestratigráficos, estructurales y metamórficos. Ellos se reflejan en una serie de parámetros que son los que habitua1ment e s e evalúan en e1 campo. La investigación utiliza técnicas geológicas básicas, adaptadas a las peculiaridades de la pizarra. Aquélla se lleva a cabo en tres fases. De cada una de las fases se presentan ejemplos. Se apuntan también algunas nuevas técnicas de investigación tomadas de la bibliografía, que podrían ser de aplicación en este campo.[Résumé] Il s'exposent les bases méthodologiques que 1es auteur s app1i quen t á 1I investigation et évaluation de gisements des ardoises pour couvertures, prisses autant de sa propre expérience que de la maigre bibliographie disponible sur le sujeto Les facteurs que controlent la qualité des gisements de la materie prime sont trois types: Litoestratiphiques, estructurales et metamórphiques. lIs se réfléchent sur une serp€ de parámetres que sont ceux que normalement s'evaluent sur le champ. L' investigation utilise les téc niques básiques, adaptées aux peculiarités de Celle-lá se mene á bien en trois phases. une des phases on presenten des exemples. On remarque aussi quelques nouvelles técniques 'investigation cherchées sur la bibliographie, qu'il pouvaient etre d'aplication sur ce champ
Intrinsic and observed dual AGN fractions from major mergers
A suite of 432 collisionless simulations of bound pairs of spiral galaxies
with mass ratios 1:1 and 3:1, and global properties consistent with the
CDM paradigm, is used to test the conjecture that major mergers fuel
the dual AGN (DAGN) of the local volume. Our analysis is based on the premise
that the essential aspects of this scenario can be captured by replacing the
physics of the central BH with restrictions on their relative separation in
phase space. We introduce several estimates of the DAGN fraction and infer
predictions for the activity levels and resolution limits usually involved in
surveys of these systems, assessing their dependence on the parameters
controlling the length of both mergers and nuclear activity. Given a set of
constraints, we find that the values adopted for some of the latter factors
often condition the outcomes from individual experiments. Still, the results do
not reveal, in general, very tight correlations, being the tendency of the
frequencies normalized to the merger time to anticorrelate with the orbital
circularity the clearest effect. In agreement with other theoretical studies,
our simulations predict intrinsic abundances of these systems that range from
few to depending on the maximum level of nuclear activity
achieved. At the same time, we show that these probabilities are reduced by
about an order of magnitude when they are filtered with the typical constraints
applied by observational studies of the DAGN fraction at low redshift. As a
whole, the results of the present work prove that the consideration of the most
common limitations involved in the detection of close active pairs at optical
wavelengths is sufficient by itself to reconcile the intrinsic frequencies
envisaged in a hierarchical universe with the small fractions of double-peaked
narrow-line systems which are often reported at kpc-scales.Comment: 24 pages, 11 figures, 3 Tables, accepted by A&
Extreme quasars at high redshift
Context:Quasars radiating at extreme Eddington ratios (xA) are likely a prime
mover of galactic evolution and have been hailed as potential distance
indicators. Their properties are still scarcely known.
Aims:We test the effectiveness of the selection criteria defined on the 4D
Eigenvector 1 (4DE1) for identifying xA sources. We provide a quantitative
description of their UV spectra in the redshift range 2<z<2.9.
Methods:19 extreme quasar candidates were identified using 4DE1 selection
criteria applied to SDSS spectra: AlIII1860/SiIII]1892>0.5 and
CIII]1909/SiIII]1892<1. The emission line spectra was studied using
multicomponent fits of deep spectroscopic observations obtained with the
OSIRIS-GTC.
Results:Spectra confirm that almost all of these quasars are xA sources with
very similar properties. We provide spectrophotometric and line profile
measurements for the SiIV1397+OIV]1402, CIV1549+HeII1640, and the 1900A blend
composed by AlIII1860, SiIII]1892, FeIII and a weak CIII]1909. The spectra can
be characterized as very low ionization (logU~-3), a condition that explains
the significant FeIII emission. CIV1549 shows low equivalent width (<30 A for
the most sources), and high or extreme blueshift amplitudes (-5000<c(1/2)<-1000
kms-1). Weak-lined quasars appear as extreme xA quasars and not as an
independent class. The CIV1549 high amplitude blueshifts coexists in all cases
save one with symmetric and narrower AlIII and SiIII] profiles. Estimates of
the Eddington ratio using the AlIII FWHM as a virial broadening estimator are
consistent with the ones of a previous xA sample.
Conclusions:It is now feasible to assemble large samples of xA quasars from
the latest data releases of the SDSS. We provide evidence that AlIII1860 could
be associated with a low-ionization virialized sub-system, supporting previous
suggestions that AlIII is a reliable virial broadening estimator.Comment: 36 pages, 31 figures, 12 tables. Manuscript accepted for publication,
A&A. Corrected titl
Spiral-like star-forming patterns in CALIFA early-type galaxies
Based on a combined analysis of SDSS imaging and CALIFA integral field
spectroscopy data, we report on the detection of faint (24 < {\mu}
mag/arcsec < 26) star-forming spiral-arm-like features in the periphery of
three nearby early-type galaxies (ETGs). These features are of considerable
interest because they document the still ongoing inside-out growth of some
local ETGs and may add valuable observational insight into the origin and
evolution of spiral structure in triaxial stellar systems. A characteristic
property of the nebular component in the studied ETGs, classified i+, is a
two-radial-zone structure, with the inner zone that displays faint
(EW(H\alpha)1{\AA}) low-ionization nuclear emission-line region (LINER)
properties, and the outer one (3{\AA}<EW(H\alpha)<~20{\AA}) HII-region
characteristics. This spatial segregation of nebular emission in two physically
distinct concentric zones calls for an examination of aperture effects in
studies of type i+ ETGs with single-fiber spectroscopic data.Comment: Accepted to A&A, 5 pages, 1 figur
Spectroscopic aperture biases in inside-out evolving early-type galaxies from CALIFA
Integral field spectroscopy studies based on CALIFA data have recently
revealed the presence of ongoing low-level star formation (SF) in the periphery
of ~10% of local early-type galaxies (ETGs), witnessing a still ongoing
inside-out galaxy growth process. A distinctive property of the nebular
component in these ETGs, classified i+, is a two-radial-zone structure, with
the inner zone displaying LINER emission with a H\alpha equivalent width
EW~1{\AA}, and the outer one (3{\AA}<EW<~20{\AA}) showing HII-region
characteristics. Using CALIFA IFS data, we empirically demonstrate that the
confinement of nebular emission to the galaxy periphery leads to a strong
aperture (or, redshift) bias in spectroscopic single-fiber studies of type i+
ETGs: At low redshift (<~0.45), SDSS spectroscopy is restricted to the inner
(SF-devoid LINER) zone, thereby leading to their erroneous classification as
"retired" galaxies (systems lacking SF and whose faint emission is powered by
pAGB stars). Only at higher z's the SDSS aperture can encompass the outer SF
zone, permitting their unbiased classification as "composite SF/LINER". We also
demonstrate that the principal effect of a decreasing aperture on the
classification of i+ ETGs via standard BPT emission-line ratios consists in a
monotonic up-right shift precisely along the upper-right wing of the "seagull"
distribution. Motivated by these insights, we also investigate theoretically
these biases in aperture-limited studies of inside-out growing galaxies as a
function of z. To this end, we devise a simple model, which involves an
outwardly propagating SF process, that reproduces the radial extent and
two-zone EW distribution of i+ ETGs. By simulating on this model the
spectroscopic SDSS aperture, we find that SDSS studies at z<~1 are
progressively restricted to the inner LINER-zone, and miss an increasingly
large portion of the H\alpha-emitting periphery.Comment: Accepted to A&A, 6 pages, 4 figure
Weyl-Underhill-Emmrich quantization and the Stratonovich-Weyl quantizer
Weyl-Underhill-Emmrich (WUE) quantization and its generalization are
considered. It is shown that an axiomatic definition of the Stratonovich-Weyl
(SW) quantizer leads to severe difficulties. Quantization on the cylinder
within the WUE formalism is discussed.Comment: 15+1 pages, no figure
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