Mittelfristige Ergebnisse der operativen Therapie bei Patienten mit Morbus Scheuermann

Retrospektive Untersuchung von 25 operativ therapierten Patienten mit hochgradigem Morbus Scheuermann über durchschnittlich 46,7 Monate. Therapieindikationen sind progrediente Kyphosierung, Schmerzen und Leidensdruck. Die durchschnittliche maximale Kyphose von 83,9° konnte auf 57,9° korrigiert werden. Innerhalb des Instrumentationsbereichs veränderte sich die Kyphose von präoperativ 72,3° auf postoperativ 47,5° und aktuell 50,8°. Der durchschnittliche Korrekturverlust lag bei 3,0°. In 11 Fällen trat eine obere junktionale Kyphose von mehr als 5° auf. Durchschnittlich lag diese bei 8,9°. Ursächlich scheinen hohe Scheitelwirbel (Th7, Th8) und eine zu kurze Instrumentationsstrecke. Die Operation führte in 59,3 % zur Schmerzreduktion. 86,4 % gaben eine Verbesserung des Selbstbildes an. 75 % der Patienten würden sich erneut operieren lassen. Die operative Korrektur beim Morbus Scheuermann führt zu hohen subjektiven Zufriedenheitswerten bei zufrieden stellenden radiometrischen Ergebnissen

Role of Lipid in Sulfite-dependent Propofol Dimerization

Background: During long-term intravenous infusions, sulfite in sulfite-containing propofol emulsions can cause the peroxidation of lipid and dimerization of propofol. This study evaluated the role of lipid in sulfite-dependent propofol dimerization by determining the effects of individual fatty acids in soybean oil emulsion and peroxidized lipids in a model system. Methods: Individual fatty acids, stearic (18:0), oleic (18:1), linoleic (18:2), linolenic (18:3), and arachidonic (20:4), were added to sulfite-containing propofol emulsion and incubated for 90 min at 37°C. Model systems containing soybean oil (100 l), water (900 l), propofol (10 mg/ml), and sulfite (0.25 mg/ml) composed of oils with different peroxide values were allowed to react for 60 min at room temperature. After the reactions, propofol dimer and propofol dimer quinone were analyzed by reversed-phase high-pressure liquid chromatography. Results: Propofol did not dimerize when added to aqueous sulfite unless soybean oil was also included. The addition of the polyunsaturated fatty acids (linoleic, linolenic, arachidonic) to sulfite-containing propofol emulsion resulted in large increases of propofol dimerization compared with stearic or oleic acid. Using biphasic mixtures of soybean oil and aqueous sulfite, propofol dimerization increased with increasing peroxide content of the oil. In propofol emulsion, lipoxidase and ferrous iron in the absence of sulfite also caused the dimerization of propofol. Conclusions: These results show that lipid can play a significant role in sulfite-dependent propofol dimerization. The relation of dimerization to polyunsaturated fatty acid and soybean oil peroxide content suggests that sulfite reacts with unsaturated lipid or peroxide-modified lipid to facilitate propofol dimerization

[Avian cytogenetics goes functional] Third report on chicken genes and chromosomes 2015

High-density gridded libraries of large-insert clones using bacterial artificial chromosome (BAC) and other vectors are essential tools for genetic and genomic research in chicken and other avian species... Taken together, these studies demonstrate that applications of large-insert clones and BAC libraries derived from birds are, and will continue to be, effective tools to aid high-throughput and state-of-the-art genomic efforts and the important biological insight that arises from them

Planck early results XV : Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources

Peer reviewe

Planck early results. XV. Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources

Spectral energy distributions (SEDs) and radio continuum spectra are presented for a northern sample of 104 extragalactic radio sources, based on the Planck Early Release Compact Source Catalogue (ERCSC) and simultaneous multifrequency data. The nine Planck frequencies, from 30 to 857 GHz, are complemented by a set of simultaneous observations ranging from radio to gamma-rays. This is the first extensive frequency coverage in the radio and millimetre domains for an essentially complete sample of extragalactic radio sources, and it shows how the individual shocks, each in their own phase of development, shape the radio spectra as they move in the relativistic jet. The SEDs presented in this paper were fitted with second and third degree polynomials to estimate the frequencies of the synchrotron and inverse Compton (IC) peaks, and the spectral indices of low and high frequency radio data, including the Planck ERCSC data, were calculated. SED modelling methods are discussed, with an emphasis on proper, physical modelling of the synchrotron bump using multiple components. Planck ERCSC data also suggest that the original accelerated electron energy spectrum could be much harder than commonly thought, with power-law index around 1.5 instead of the canonical 2.5. The implications of this are discussed for the acceleration mechanisms effective in blazar shocks. Furthermore in many cases the Planck data indicate that gamma-ray emission must originate in the same shocks that produce the radio emission

Measurement of ϒ production in pp collisions at √s = 2.76 TeV

The production of ϒ(1S), ϒ(2S) and ϒ(3S) mesons decaying into the dimuon final state is studied with the LHCb detector using a data sample corresponding to an integrated luminosity of 3.3 pb−1 collected in proton–proton collisions at a centre-of-mass energy of √s = 2.76 TeV. The differential production cross-sections times dimuon branching fractions are measured as functions of the ϒ transverse momentum and rapidity, over the ranges pT < 15 GeV/c and 2.0 < y < 4.5. The total cross-sections in this kinematic region, assuming unpolarised production, are measured to be σ (pp → ϒ(1S)X) × B ϒ(1S)→μ+μ− = 1.111 ± 0.043 ± 0.044 nb, σ (pp → ϒ(2S)X) × B ϒ(2S)→μ+μ− = 0.264 ± 0.023 ± 0.011 nb, σ (pp → ϒ(3S)X) × B ϒ(3S)→μ+μ− = 0.159 ± 0.020 ± 0.007 nb, where the first uncertainty is statistical and the second systematic