5,072 research outputs found
Environmental Impact on the Southeast Limb of the Cygnus Loop
We analyze observations from the Chandra X-ray Observatory of the southeast
knot of the Cygnus Loop supernova remnant. In this region, the blast wave
propagates through an inhomogeneous environment. Extrinsic differences and
subsequent multiple projections along the line of sight rather than intrinsic
shock variations, such as fluid instabilities, account for the apparent
complexity of the images. Interactions between the supernova blast wave and
density enhancements of a large interstellar cloud can produce the
morphological and spectral characteristics. Most of the X-ray flux arises in
such interactions, not in the diffuse interior of the supernova remnant.
Additional observations at optical and radio wavelengths support this account
of the existing interstellar medium and its role in shaping the Cygnus Loop,
and they demonstrate that the southeast knot is not a small cloud that the
blast wave has engulfed. These data are consistent with rapid equilibration of
electron and ion temperatures behind the shock front, and the current blast
wave velocity v_{bw} approx 330 km/s. Most of this area does not show strong
evidence for non-equilibrium ionization conditions, which may be a consequence
of the high densities of the bright emission regions.Comment: To appear in ApJ, April 1, 200
Can guidelines improve referral to elective surgical specialties for adults? A systematic review
Aim To assess effectiveness of guidelines for referral for
elective surgical assessment.
Method Systematic review with descriptive synthesis.
Data sources Medline, EMBASE, CINAHL and Cochrane
database up to 2008. Hand searches of journals and
websites.
Selection of studies Studies evaluated guidelines for
referral from primary to secondary care, for elective
surgical assessment for adults.
Outcome measures Appropriateness of referral (usually
measured as guideline compliance) including clinical
appropriateness, appropriateness of destination and of
pre-referral management (eg, diagnostic investigations),
general practitioner knowledge of referral
appropriateness, referral rates, health outcomes and
costs.
Results 24 eligible studies (5 randomised control trials,
6 cohort, 13 case series) included guidelines from UK,
Europe, Canada and the USA for referral for
musculoskeletal, urological, ENT, gynaecology, general
surgical and ophthalmological conditions. Interventions
varied from complex (“one-stop shops”) to simple
guidelines. Four randomized control trials reported
increases in appropriateness of pre-referral care
(diagnostic investigations and treatment). No evidence
was found for effects on practitioner knowledge. Mixed
evidence was reported on rates of referral and costs
(rates and costs increased, decreased or stayed the
same). Two studies reported on health outcomes finding
no change.
Conclusions Guidelines for elective surgical referral can
improve appropriateness of care by improving prereferral
investigation and treatment, but there is no
strong evidence in favour of other beneficial effects
Binaries and the dynamical mass of star clusters
The total mass of a distant star cluster is often derived from the virial
theorem, using line-of-sight velocity dispersion measurements and half-light
radii, under the implicit assumption that all stars are single (although it is
known that most stars form part of binary systems). The components of binary
stars exhibit orbital motion, which increases the measured velocity dispersion,
resulting in a dynamical mass overestimation. In this article we quantify the
effect of neglecting the binary population on the derivation of the dynamical
mass of a star cluster. We find that the presence of binaries plays an
important role for clusters with total mass M < 10^5 Msun; the dynamical mass
can be significantly overestimated (by a factor of two or more). For the more
massive clusters, with Mcl > 10^5 Msun, binaries do not affect the dynamical
mass estimation significantly, provided that the cluster is significantly
compact (half-mass radius < 5 pc).Comment: Comments: 2 pages. Conference proceedings for IAUS246 'Dynamical
Evolution of Dense Stellar Systems', ed. E. Vesperini (Chief Editor), M.
Giersz, A. Sills, Capri, Sept. 200
Optimal Occulter Design for Finding Extrasolar Planets
One proposed method for finding terrestrial planets around nearby stars is to
use two spacecraft--a telescope and a specially shaped occulter that is
specifically designed to prevent all but a tiny fraction of the starlight from
diffracting into the telescope. As the cost and observing cadence for such a
mission will be driven largely by the separation between the two spacecraft, it
is critically important to design an occulter that can meet the observing goals
while flying as close to the telescope as possible. In this paper, we explore
this tradeoff between separation and occulter diameter. More specifically, we
present a method for designing the shape of the outer edge of an occulter that
is as small as possible and gives a shadow that is deep enough and large enough
for a 4m telescope to survey the habitable zones of many stars for Earth-like
planets. In particular, we show that in order for a 4m telescope to detect in
broadband visible light a planet 0.06 arcseconds from a star shining
times brighter than the planet requires a specially-shaped occulter 50m in
diameter positioned about km in front of the telescope.Comment: 14 pages, 4 figures, 15 subfigure
What's age got to do with it? Supreme Court appointees and the long run location of the Supreme Court median justice
For approximately the past forty years, Republican Presidents have appointed younger Justices than have Democratic Presidents. Depending on how one does the accounting, the average age difference will vary, but will not go away. This Article posits that Republicans appointing younger justices than Democrats may have caused a rightward shift in the Supreme Court. We use computer simulations to show that if the trend continues the rightward shift will likely increase. We also produce some very rough estimates of the size of the ideological shift, contingent on the size of the age differential. In addition, we show that the Senate’s role in confirming nominated Justices has a significant moderating effect on the shift. Last, we consider the interaction between our results and the oft-proposed eighteen year staggered terms for Supreme Court Justices. We show that such an institutional change would almost completely wipe out the ideological effect of one Party appointing younger Justices
First exit times and residence times for discrete random walks on finite lattices
In this paper, we derive explicit formulas for the surface averaged first
exit time of a discrete random walk on a finite lattice. We consider a wide
class of random walks and lattices, including random walks in a non-trivial
potential landscape. We also compute quantities of interest for modelling
surface reactions and other dynamic processes, such as the residence time in a
subvolume, the joint residence time of several particles and the number of hits
on a reflecting surface.Comment: 19 pages, 2 figure
Construction of the factorized steady state distribution in models of mass transport
For a class of one-dimensional mass transport models we present a simple and
direct test on the chipping functions, which define the probabilities for mass
to be transferred to neighbouring sites, to determine whether the stationary
distribution is factorized. In cases where the answer is affirmative, we
provide an explicit method for constructing the single-site weight function. As
an illustration of the power of this approach, previously known results on the
Zero-range process and Asymmetric random average process are recovered in a few
lines. We also construct new models, namely a generalized Zero-range process
and a binomial chipping model, which have factorized steady states.Comment: 6 pages, no figure
- …