3,941 research outputs found
State Campaign Finance Law: An Overview and a Call for Reform
Trabajo académicoEl objetivo del estudio es determinar la relación entre la preoxigenación subóptima y la morbimortalidad en pacientes con manejo de vía aérea en el servicio de emergencia del Hospital Nacional Arzobispo Loayza en el 2018. Para ello se plantea un estudio observacional, analítico y prospectivo; la muestra estará constituida por 90 pacientes con manejo de vía aérea en el servicio de emergencia del Hospital Nacional Arzobispo Loayza durante el periodo julio – diciembre de 2018. La técnica de recolección será observación y el instrumento será una ficha de recolección y una lista de verificación. El análisis de los datos se realizará en el programa estadístico Statistical Package for the Social Sciences (SPSS) versión 23. Para la relación entre la preoxigenación subóptima y morbilidad /mortalidad se aplicará la prueba Chi-Cuadrado, considerando un nivel de significancia del 5%. Es importante y relevante desarrollar el estudio ya que permitirá un mayor conocimiento sobre el manejo más adecuado de las vías aéreas en pacientes atendidos en el servicio de emergencia del Hospital Nacional Arzobispo Loayza
Missouri\u27s Hearsay Exception Statute for Victims of Child Sexual Abuse: Upheld by the Missouri Supreme Court
Detecting circumbinary planets using eclipse timing of binary stars - numerical simulations
The presence of a body in an orbit around a close eclipsing binary star
manifests itself through the light time effect influencing the observed times
of eclipses as the close binary and the circumbinary companion both move around
the common centre of mass. This fact combined with the periodicity with which
the eclipses occur can be used to detect the companion. Given a sufficient
precision of the times of eclipses, the eclipse timing can be employed to
detect substellar or even planetary mass companions.
The main goal of the paper is to investigate the potential of the photometry
based eclipse timing of binary stars as a method of detecting circumbinary
planets. In the models we assume that the companion orbits a binary star in a
circular Keplerian orbit. We analyze both the space and ground based photometry
cases. In particular, we study the usefulness of the on-going COROT and Kepler
missions in detecting circumbinary planets. We also explore the relations
binding the planet discovery space with the physical parameters of the binaries
and the geometrical parameters of their light curves. We carry out detailed
numerical simulations of the eclipse timing by employing a relatively realistic
model of the light curves of eclipsing binary stars. We study the influence of
the white and red photometric noises on the timing precision. We determine the
sensitivity of the eclipse timing technique to circumbinary planets for the
ground and space based photometric observations. We provide suggestions for the
best targets, observing strategies and instruments for the eclipse timing
method. Finally, we compare the eclipse timing as a planet detection method
with the radial velocities and astrometry.Comment: 9 pages, 15 figures, accepted for publication in MNRA
CoRoT's first seven planets: An overview
The up to 150 day uninterrupted high-precision photometry of about 100000
stars - provided so far by the exoplanet channel of the CoRoT space telescope -
gave a new perspective on the planet population of our galactic neighbourhood.
The seven planets with very accurate parameters widen the range of known planet
properties in almost any respect. Giant planets have been detected at low
metallicity, rapidly rotating and active, spotted stars. CoRoT-3 populated the
brown dwarf desert and closed the gap of measured physical properties between
standard giant planets and very low mass stars. CoRoT extended the known range
of planet masses down to 5 Earth masses and up to 21 Jupiter masses, the radii
to less than 2 Earth radii and up to the most inflated hot Jupiter found so
far, and the periods of planets discovered by transits to 9 days. Two CoRoT
planets have host stars with the lowest content of heavy elements known to show
a transit hinting towards a different planet-host-star-metallicity relation
then the one found by radial-velocity search programs. Finally the properties
of the CoRoT-7b prove that terrestrial planets with a density close to Earth
exist outside the Solar System. The detection of the secondary transit of
CoRoT-1 at the -level and the very clear detection of the 1.7 Earth
radii of CoRoT-7b at relative flux are promising evidence of
CoRoT being able to detect even smaller, Earth sized planets.Comment: 8 pages, 19 figures and 3 table
Network Model of the CPE
Analysis of fractal systems (i.e. systems described by fractional differential equations) necessitates to create an electrical analog model of a crucial subsystem called Constant Phase Element (CPE). The paper describes a possible realization of such a model, that is quite simple and in spite of its simplicity makes it possible to simulate the properties of ideal CPEs. The paper also deals with the effect of component tolerances on the resultant responses of the model and describes several typical model applications
Where are the Uranus Trojans?
The area of stable motion for fictitious Trojan asteroids around Uranus'
equilateral equilibrium points is investigated with respect to the inclination
of the asteroid's orbit to determine the size of the regions and their shape.
For this task we used the results of extensive numerical integrations of orbits
for a grid of initial conditions around the points L4 and L5, and analyzed the
stability of the individual orbits. Our basic dynamical model was the Outer
Solar System (Jupiter, Saturn, Uranus and Neptune). We integrated the equations
of motion of fictitious Trojans in the vicinity of the stable equilibrium
points for selected orbits up to the age of the Solar system of 5 billion
years. One experiment has been undertaken for cuts through the Lagrange points
for fixed values of the inclinations, while the semimajor axes were varied. The
extension of the stable region with respect to the initial semimajor axis lies
between 19.05 < a < 19.3 AU but depends on the initial inclination. In another
run the inclination of the asteroids' orbit was varied in the range 0 < i < 60
and the semimajor axes were fixed. It turned out that only four 'windows' of
stable orbits survive: these are the orbits for the initial inclinations 0 < i
< 7, 9 < i < 13, 31 < i < 36 and 38 < i < 50. We postulate the existence of at
least some Trojans around the Uranus Lagrange points for the stability window
at small and also high inclinations.Comment: 15 pages, 12 figures, submitted to CMD
Clark Canyon Recreation Survey: 2003-2004
This report summarizes a study of recreation use on Clark Canyon Reservoir and Barretts Campground from May 24, 2003 to February 29, 2004
Visitor Profile of Snowcoach Passengers in West Yellowstone, MT
The purpose of this study was to provide an understanding of who is using the West Yellowstone snowcoach, why they are visiting, and what encouraged them to take a snowcoach trip
Metabolismus und Toxizitaet therapeutischer Chelatbildner. 8. Mitteilung: Ausscheidung von Natrium, Kalium, Magnesium und Zink
- …