364 research outputs found
DER EINSATZ HOLOGRAPHISCHER VERFAHREN IN DER MEDIZIN
The author reviews present and future medical applications - both in medical research and clinicaI practice - of hoIography and hoIography-based procedures, incIuding 3-D images of high depth
of focus in the object space, holography with waves outside the visible range (microwaves, infrated,
uItrasonics, X-rays), holographic analysis of movements, holographic endoscopy and military appIi-
cations ("Star Wars Medicine")
Worte der Trauer gesprochen an den Särgen des Fßrsten von Lichnowsky und des Generals von Auerswald, deutscher Reichstagsmitglieder
The Birth of High Mass Stars: Accretion and/or Mergers?
The observational consequences of the merger scenario for massive star
formation are explored and contrasted with the gradual accumulation of mass by
accretion. Protostellar mergers may produce high luminosity infrared flares
lasting years to centuries followed by a luminosity decline on the
Kelvin-Helmholtz time-scale of the merger product. Mergers may be surrounded by
thick tori of expanding debris, impulsive wide-angle outflows, and shock
induced maser and radio continuum emission. Collision products are expected to
have fast stellar rotation and a large multiplicity fraction. Close encounters
or mergers will produce circumstellar debris disks with an orientation that
differs form that of a pre-existing disk. The extremely rare merger of two
stars close to the upper-mass end of the IMF may be a possible pathway to
hypernova generated gamma-ray bursters. While accretional growth can lead to
the formation of massive stars in isolation or in loose clusters, mergers can
only occur in high-density cluster environments. It is proposed that the
outflow emerging from the OMC1 core in the Orion molecular cloud was produced
by a protostellar merger that released between to ergs less
than a thousand years ago
Submillimeter Emission from Water in the W3 Region
We have mapped the submillimeter emission from the 1(10)-1(01) transition of
ortho-water in the W3 star-forming region. A 5'x5' map of the W3 IRS4 and W3
IRS5 region reveals strong water lines at half the positions in the map. The
relative strength of the Odin lines compared to previous observations by SWAS
suggests that we are seeing water emission from an extended region. Across much
of the map the lines are double-peaked, with an absorption feature at -39 km/s;
however, some positions in the map show a single strong line at -43 km/s. We
interpret the double-peaked lines as arising from optically thick,
self-absorbed water emission near the W3 IRS5, while the narrower blue-shifted
lines originate in emission near W3 IRS4. In this model, the unusual appearance
of the spectral lines across the map results from a coincidental agreement in
velocity between the emission near W3 IRS4 and the blue peak of the more
complex lines near W3 IRS5. The strength of the water lines near W3 IRS4
suggests we may be seeing water emission enhanced in a photon-dominated region.Comment: Accepted to A&A Letters as part of the special Odin issue; 4 page
Exoplanet Characterization and the Search for Life
Over 300 extrasolar planets (exoplanets) have been detected orbiting nearby
stars. We now hope to conduct a census of all planets around nearby stars and
to characterize their atmospheres and surfaces with spectroscopy. Rocky planets
within their star's habitable zones have the highest priority, as these have
the potential to harbor life. Our science goal is to find and characterize all
nearby exoplanets; this requires that we measure the mass, orbit, and
spectroscopic signature of each one at visible and infrared wavelengths. The
techniques for doing this are at hand today. Within the decade we could answer
long-standing questions about the evolution and nature of other planetary
systems, and we could search for clues as to whether life exists elsewhere in
our galactic neighborhood.Comment: 7 pages, 2 figures, submitted to Astro2010 Decadal Revie
Control of star formation by supersonic turbulence
Understanding the formation of stars in galaxies is central to much of modern
astrophysics. For several decades it has been thought that stellar birth is
primarily controlled by the interplay between gravity and magnetostatic
support, modulated by ambipolar diffusion. Recently, however, both
observational and numerical work has begun to suggest that support by
supersonic turbulence rather than magnetic fields controls star formation. In
this review we outline a new theory of star formation relying on the control by
turbulence. We demonstrate that although supersonic turbulence can provide
global support, it nevertheless produces density enhancements that allow local
collapse. Inefficient, isolated star formation is a hallmark of turbulent
support, while efficient, clustered star formation occurs in its absence. The
consequences of this theory are then explored for both local star formation and
galactic scale star formation. (ABSTRACT ABBREVIATED)Comment: Invited review for "Reviews of Modern Physics", 87 pages including 28
figures, in pres
Monitoring Procalcitonin in Febrile Neutropenia: What Is Its Utility for Initial Diagnosis of Infection and Reassessment in Persistent Fever?
Background: Management of febrile neutropenic episodes (FE) is challenged by lacking microbiological and clinical documentation of infection. We aimed at evaluating the utility of monitoring blood procalcitonin (PCT) in FE for initial diagnosis of infection and reassessment in persistent fever.Methods: PCT kinetics was prospectively monitored in 194 consecutive FE (1771 blood samples): 65 microbiologically documented infections (MDI, 33.5%; 49 due to non-coagulase-negative staphylococci, non-CNS), 68 clinically documented infections (CDI, 35%; 39 deep-seated), and 61 fever of unexplained origin (FUO, 31.5%).Results: At fever onset median PCT was 190 pg/mL (range 30-26'800), without significant difference among MDI, CDI and FUO. PCT peak occurred on day 2 after onset of fever: non-CNS-MDI/deep-seated-CDI (656, 80-86350) vs. FUO (205, 33-771; p<0.001). PCT >500 pg/mL distinguished non-CNS-MDI/deep-seated-CDI from FUO with 56% sensitivity and 90% specificity. PCT was >500 pg/ml in only 10% of FUO (688, 570-771). A PCT peak >500 pg/mL (1196, 524-11950) occurred beyond 3 days of persistent fever in 17/21 (81%) invasive fungal diseases (IFD). This late PCT peak identified IFD with 81% sensitivity and 57% specificity and preceded diagnosis according to EORTC-MSG criteria in 41% of cases. In IFD responding to therapy, median days to PCT <500 pg/mL and defervescence were 5 (1-23) vs. 10 (3-22; p = 0.026), respectively.Conclusion: While procalcitonin is not useful for diagnosis of infection at onset of neutropenic fever, it may help to distinguish a minority of potentially severe infections among FUOs on day 2 after onset of fever. In persistent fever monitoring procalcitonin contributes to early diagnosis and follow-up of invasive mycose
Performance of the CMS Cathode Strip Chambers with Cosmic Rays
The Cathode Strip Chambers (CSCs) constitute the primary muon tracking device
in the CMS endcaps. Their performance has been evaluated using data taken
during a cosmic ray run in fall 2008. Measured noise levels are low, with the
number of noisy channels well below 1%. Coordinate resolution was measured for
all types of chambers, and fall in the range 47 microns to 243 microns. The
efficiencies for local charged track triggers, for hit and for segments
reconstruction were measured, and are above 99%. The timing resolution per
layer is approximately 5 ns
Performance and Operation of the CMS Electromagnetic Calorimeter
The operation and general performance of the CMS electromagnetic calorimeter
using cosmic-ray muons are described. These muons were recorded after the
closure of the CMS detector in late 2008. The calorimeter is made of lead
tungstate crystals and the overall status of the 75848 channels corresponding
to the barrel and endcap detectors is reported. The stability of crucial
operational parameters, such as high voltage, temperature and electronic noise,
is summarised and the performance of the light monitoring system is presented
Primary versus secondary source of data in observational studies and heterogeneity in meta-analyses of drug effects: a survey of major medical journals
The data from individual observational studies included in meta-analyses of drug effects are collected either from ad hoc methods (i.e. "primary data") or databases that were established for non-research purposes (i.e. "secondary data"). The use of secondary sources may be prone to measurement bias and confounding due to over-the-counter and out-of-pocket drug consumption, or non-adherence to treatment. In fact, it has been noted that failing to consider the origin of the data as a potential cause of heterogeneity may change the conclusions of a meta-analysis. We aimed to assess to what extent the origin of data is explored as a source of heterogeneity in meta-analyses of observational studies.publishe
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