1,819 research outputs found
Gravitational wave background from binary systems
Basic aspects of the background of gravitational waves and its mathematical
characterization are reviewed. The spectral energy density parameter
, commonly used as a quantifier of the background, is derived for an
ensemble of many identical sources emitting at different times and locations.
For such an ensemble, is generalized to account for the duration of
the signals and of the observation, so that one can distinguish the resolvable
and unresolvable parts of the background. The unresolvable part, often called
confusion noise or stochastic background, is made by signals that cannot be
either individually identified or subtracted out of the data. To account for
the resolvability of the background, the overlap function is introduced. This
function is a generalization of the duty cycle, which has been commonly used in
the literature, in some cases leading to incorrect results. The spectra
produced by binary systems (stellar binaries and massive black hole binaries)
are presented over the frequencies of all existing and planned detectors. A
semi-analytical formula for is derived in the case of stellar
binaries (containing white dwarfs, neutron stars or stellar-mass black holes).
Besides a realistic expectation of the level of background, upper and lower
limits are given, to account for the uncertainties in some astrophysical
parameters such as binary coalescence rates. One interesting result concerns
all current and planned ground-based detectors (including the Einstein
Telescope). In their frequency range, the background of binaries is resolvable
and only sporadically present. In other words, there is no stochastic
background of binaries for ground-based detectors.Comment: 30 pages, 16 figure
CONTINUOUS EMISSION, LOWERING OF THE IONIZATION POTENTIAL AND TOTAL EXCITATION CROSS-SECTIONS OF AN ATMOSPHERIC THERMAL PLASMA
Structure of Supergiant Shells in the Large Magellanic Cloud
Nine supergiant shells (SGSs) have been identified in the Large Magellanic
Cloud (LMC) based on H-alpha images, and twenty-three SGSs have been reported
based on HI 21-cm line observations, but these sets do not always identify the
same structures. We have examined the physical structure of the optically
identified SGSs using HI channel maps and P-V diagrams to analyze the gas
kinematics. There is good evidence for seven of the nine optically identified
SGSs to be true shells. Of these seven H-alpha SGSs, four are the ionized inner
walls of HI SGSs, while three are an ionized portion of a larger and more
complex HI structure. All of the H-alpha SGSs are identified as such because
they have OB associations along the periphery or in the center, with younger OB
associations more often found along the periphery. After roughly 12 Myrs, if no
new OB associations have been formed a SGS will cease to be identifiable at
visible wavelengths. Thus, the presence and location of ionizing sources is the
main distinction between shells seen only in HI and those also seen in H-alpha.
Based on our analysis, H-alpha observations alone cannot unambiguously identify
SGSs, especially in distant galaxies.Comment: 26 pages, 16 figures, accepted for publication in the Astrophysical
Journal Supplemen
The implementation of e-learning in the continuous training of the military of the Republican National Guard. Case study: Lisbon Territorial Command
The training needs felt in the professional path of the military of the Republican National
Guard, associated with the potential of using new technologies is the core of this investigation.
Training is one of the great challenges that organizations currently face and, in the National
Republican Guard, it plays a fundamental role in the service provided by the Institution, making it
clear the high importance of acquiring and maintaining knowledge and skills for the performance on
several roles in the organization. The present investigation aims to determine the importance of the
e-Learning tool for the continuous training of the soldiers of the National Republican Guard. In this
context, it is intended to characterize the importance of continuous training whose objective is to
identify and analyze the consequences of the tool, as well as to identify the impact of the use of new
technologies in the training of the institution's military, according to a case study in the Lisbon
Territorial Command. The method that supports the investigation is the deductive method, which is
based on a logic from the general to the particular. In order to achieve the defined objectives, we
opted for interviews and a questionnaire survey, complemented with a documentary analysis resulting
from bibliographic research and institutional documents. Thus, it appears that continuous training has
a high importance for the professional development of the military, since it promotes quality in the
service provided, positively affecting the daily activities of the military, increasing individual success
and, consequently, organizational success . It is concluded that e-Learning represents an asset for
continuous training, since it is a catalyst for the potential of the institution's human resources.info:eu-repo/semantics/publishedVersio
Gravitational wave background from rotating neutron stars
The background of gravitational waves produced by the ensemble of rotating
neutron stars (which includes pulsars, magnetars and gravitars) is
investigated. A formula for \Omega(f) (commonly used to quantify the
background) is derived, properly taking into account the time evolution of the
systems since their formation until the present day. Moreover, the formula
allows one to distinguish the different parts of the background: the
unresolvable (which forms a stochastic background) and the resolvable. Several
estimations of the background are obtained, for different assumptions on the
parameters that characterize neutron stars and their population. In particular,
different initial spin period distributions lead to very different results. For
one of the models, with slow initial spins, the detection of the background can
be rejected. However, other models do predict the detection of the background
by the future ground-based gravitational wave detector ET. A robust upper limit
for the background of rotating neutron stars is obtained; it does not exceed
the detection threshold of two cross-correlated Advanced LIGO interferometers.
If gravitars exist and constitute more than a few percent of the neutron star
population, then they produce an unresolvable background that could be detected
by ET. Under the most reasonable assumptions on the parameters characterizing a
neutron star, the background is too faint. Previous papers have suggested
neutron star models in which large magnetic fields (like the ones that
characterize magnetars) induce big deformations in the star, which produce a
stronger emission of gravitational radiation. Considering the most optimistic
(in terms of the detection of gravitational waves) of these models, an upper
limit for the background produced by magnetars is obtained; it could be
detected by ET, but not by BBO or DECIGO.Comment: 25 pages, 15 figure
24-hour Heart Rate is Related to Lower Extremity Venous Vascular Function in Persons with Paraplegia
Please refer to the pdf version of the abstract located adjacent to the title
Resistance to ceratocystis wilt (Ceratocystis fimbriata) in parents and progenies of Eucalyptus grandis x E. urophylla.
Ceratocystis wilt, caused by Ceratocystis fimbriata, is one ofthe most damaging diseases in eucalyptus plantations worldwide. Although there are resistant genotypes, the genetic basis of resistance is still poorly understood. In this paper we studied the resistance leveI by a stem inoculation experiment of genotypes of Eucalyptus grandis and E. urophylla and estimated the heritability and gains of selection in families derived from controlled interspecific crosses. In both species, highly resistant as well as highly susceptible genotypes to Ceratocystis wilt were found. Out of 21 parents assessed, twelve were resistant and nine susceptible. Estimates of individual narrow (50%) and broad (59%) sense heritability suggested a high degree of genetic control and low allelic dominance of the trait. There was great genetic variation among and within families, a fact that contributes to high heritability and genetic gain. A genetic gain in lesion size of up to -74.4 % was obtained from selection of the 50 best clones in the evaluated families, i.e., the mean lesion length in the progeny population can be reduced by 74,4%
HII Shells Surrounding Wolf-Rayet stars in M31
We present the results of an ongoing investigation to provide a detailed view
of the processes by which massive stars shape the surrounding interstellar
medium (ISM), from pc to kpc scales. In this paper we have focused on studying
the environments of Wolf-Rayet (WR) stars in M31 to find evidence for WR
wind-ISM interactions, through imaging ionized hydrogen nebulae surrounding
these stars.
We have conducted a systematic survey for HII shells surrounding 48 of the 49
known WR stars in M31. There are 17 WR stars surrounded by single shells, or
shell fragments, 7 stars surrounded by concentric limb brightened shells, 20
stars where there is no clear physical association of the star with nearby
H-alpha emission, and 4 stars which lack nearby H-alpha emission. For the 17+7
shells above, there are 12 which contain one or two massive stars (including a
WR star) and that are <=40 pc in radius. These 12 shells may be classical WR
ejecta or wind-blown shells. Further, there may be excess H-alpha point source
emission associated with one of the 12 WR stars surrounded by putative ejecta
or wind-blown shells. There is also evidence for excess point source emission
associated with 11 other WR stars. The excess emission may arise from
unresolved circumstellar shells, or within the extended outer envelopes of the
stars themselves.
In a few cases we find clear morphological evidence for WR shells interacting
with each other. In several H-alpha images we see WR winds disrupting, or
punching through, the walls of limb-brightened HII shells.Comment: 20 pages, 4 figures (in several parts: some .jpg and others .ps),
accepted to AJ (appearing Oct, 1999
Inhibition of JAK3 with a novel, selective and orally active small molecule induces therapeutic response in T-cell malignancies.
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