384 research outputs found
Lipopolysaccharide exacerbates functional and inflammatory responses to ovalbumin and decreases sensitivity to inhaled fluticasone propionate in a guinea-pig model of asthma
Background and Purpose Asthma exacerbations contribute to corticosteroid insensitivity. Lipopolysaccharide (LPS) is ubiquitous in the environment. It causes bronchoconstriction and airways inflammation and may therefore exacerbate allergen responses. This study examined whether LPS and ovalbumin co-administration could exacerbate the airways inflammatory and functional responses to ovalbumin in conscious guinea-pigs and whether these exacerbated responses were insensitive to inhaled corticosteroid treatment with fluticasone propionate. Experimental Approach Guinea-pigs were sensitized and challenged with ovalbumin and airways function recorded as specific airways conductance (sGaw) by whole body plethysmography. Airways inflammation was measured from lung histology and bronchoalveolar lavage. Airways hyperreactivity (AHR) to inhaled histamine was examined 24h after ovalbumin. LPS was inhaled alone or 24 or 48 hours before ovalbumin and combined with ovalbumin. Fluticasone propionate (0.05, 0.1, 0.5 or 1mg/ml) or vehicle (ethanol:DMSO:saline 30:30:40) was nebulised for 15 minutes twice daily for 6 days before ovalbumin or LPS exposure. Key Results Ovalbumin inhalation caused early (EAR) and late asthmatic responses (LAR), airways hypereactivity to histamine and influx of inflammatory cells into the lungs. LPS 48 hours before and co-administered with ovalbumin exacerbated the response with increased length of the EAR, prolonged response to histamine and elevated inflammatory cells. FP 0.5 and 1mg/ml reduced the LAR, AHR and cell influx with ovalbumin alone, but was ineffective when guinea-pigs were exposed to LPS before and with ovalbumin. Conclusions and Implications LPS exposure exacerbates airways inflammatory and functional responses to allergen inhalation and decreases corticosteroid sensitivity. Its widespread presence in the environment could contribute to asthma exacerbations and corticosteroid insensitivity in humans
Accidental hepatic artery ligation in humans
Despite the vast amount of information from experimental animals, it has been difficult to obtain a clear-cut picture of the effects of ligation of the hepatic artery in humans with relatively normal livers. The last complete review of this subject in 1933 indicated that a mortality in excess of 50 per cent could be expected in non-cirrhotic patients with injury of the hepatic artery or its principal branches. Five cases of dearterialization of the normal human liver have been observed. These were due to accidental interruption of the right hepatic artery in four and the proper hepatic artery in one. The injured vessel was repaired in one case and ligated in the others. In four of the five patients the vascular disruption was the sole injury. In the other the common bile duct was also lacerated. There was no evidence of hepatic necrosis in any case although one patient died from complications of common duct repair. Transient changes in SGOT and temporary low grade bilirubinemia were commonly noted. In addition, all cases of ligation of the hepatic artery reported since 1933 have been compiled. On the basis of reviewed, as well as the presently reported cases, it is concluded that ligation of the hepatic artery or one of its branches in the patient with relatively normal hepatic function is not ordinarily fatal in the otherwise uncomplicated case. Adequate perfusion of the liver can usually be provided by the remaining portal venous flow and whatever arterial collaterals are present, unless additional factors further reduce the portal venous flow or increase hepatic oxygen need. These factors include fever, shock and anoxia. The key to therapy in unreconstructed injuries to the hepatic artery is avoidance of these secondary influences. © 1964
Non Linear Current Response of a Many-Level Tunneling System: Higher Harmonics Generation
The fully nonlinear response of a many-level tunneling system to a strong
alternating field of high frequency is studied in terms of the
Schwinger-Keldysh nonequilibrium Green functions. The nonlinear time dependent
tunneling current is calculated exactly and its resonance structure is
elucidated. In particular, it is shown that under certain reasonable conditions
on the physical parameters, the Fourier component is sharply peaked at
, where is the spacing between
two levels. This frequency multiplication results from the highly nonlinear
process of photon absorption (or emission) by the tunneling system. It is
also conjectured that this effect (which so far is studied mainly in the
context of nonlinear optics) might be experimentally feasible.Comment: 28 pages, LaTex, 7 figures are available upon request from
[email protected], submitted to Phys.Rev.
Fast variability from black-hole binaries
Currently available information on fast variability of the X-ray emission
from accreting collapsed objects constitutes a complex phenomenology which is
difficult to interpret. We review the current observational standpoint for
black-hole binaries and survey models that have been proposed to interpret it.
Despite the complex structure of the accretion flow, key observational
diagnostics have been identified which can provide direct access to the
dynamics of matter motions in the close vicinity of black holes and thus to the
some of fundamental properties of curved spacetimes, where strong-field general
relativistic effects can be observed.Comment: 20 pages, 11 figures. Accepted for publication in Space Science
Reviews. Also to appear in hard cover in the Space Sciences Series of ISSI
"The Physics of Accretion onto Black Holes" (Springer Publisher
Jupiter's X-ray Emission 2007 Part 2:Comparisons with UV and Radio Emissions and In-Situ Solar Wind Measurements
We compare Chandra and XMMâNewton Xâray observations of Jupiter during 2007 with a rich multiâinstrument dataset including: upstream inâsitu solar wind measurements from the New Horizons spacecraft, radio emissions from the Nançay Decametric Array and Wind/Waves, and UV observations from the Hubble Space Telescope. New Horizons data revealed two corotating interaction regions (CIRs) impacted Jupiter during these observations. NonâIo decametric bursts and UV emissions brightened together and varied in phase with the CIRs. We characterise 3 types of Xâray aurorae: hard Xâray bremsstrahlung main emission, pulsed/flared soft Xâray emissions and a newly identified dim flickering (varying on shortâtimescales, but quasiâcontinuously present) aurora. For most observations, the Xâray aurorae were dominated by pulsed/flaring emissions, with ion spectral lines that were best fit by Iogenic plasma. However, the brightest Xâray aurora was coincident with a magnetosphere expansion. For this observation, the aurorae were produced by both flickering emission and erratic pulses/flares. Auroral spectral models for this observation required the addition of solar wind ions to attain good fits, suggesting solar wind entry into the outer magnetosphere or directly into the pole for this particularly bright observation. Xâray bremsstrahlung from high energy electrons was only bright for one observation, which was during a forward shock. This bremsstrahlung was spatially coincident with bright UV main emission (power> 1TW) and Xâray ion spectral line dusk emission, suggesting closening of upward and downward current systems during the shock. Otherwise, the bremsstrahlung was dim and UV main emission power was also lower(<700 GW), suggesting their power scaled together
Jupiter's X-ray Emission During Solar Minimum
The 2007â2009 solar minimum was the longest of the space age. We present the first of two companion papers on Chandra and XMMâNewton Xâray campaigns of Jupiter through FebruaryâMarch 2007. We find that low solar Xâray flux during solar minimum causes Jupiter's equatorial regions to be exceptionally Xâray dim (0.21 GW at minimum; 0.76 GW at maximum). While the Jovian equatorial emission varies with solar cycle, the aurorae have comparably bright intervals at solar minimum and maximum. We apply atomic charge exchange models to auroral spectra and find that iogenic plasma of sulphur and oxygen ions provides excellent fits for XMMâNewton observations. The fitted spectral S:O ratios of 0.4â1.3 are in good agreement with in situ magnetospheric S:O measurements of 0.3â1.5, suggesting that the ions that produce Jupiter's Xâray aurora predominantly originate inside the magnetosphere. The aurorae were particularly bright on 24â25 February and 8â9 March, but these two observations exhibit very different spatial, spectral, and temporal behavior; 24â25 February was the only observation in this campaign with significant hard Xâray bremsstrahlung from precipitating electrons, suggesting this may be rare. For 8â9 March, a bremsstrahlung component was absent, but bright oxygen O6+ lines and bestâfit models containing carbon, point to contributions from solar wind ions. This contribution is absent in the other observations. Comparing simultaneous Chandra ACIS and XMMâNewton EPIC spectra showed that ACIS systematically underreported 0.45â to 0.6âkeV Jovian emission, suggesting quenching may be less important for Jupiter's atmosphere than previously thought. We therefore recommend XMMâNewton for spectral analyses and quantifying opacity/quenching effects
Regional Adoption of Business-to-Business Electronic Commerce in China: Role of E-Readiness
Adoption of B2B e-commerce is a powerful driver of economic success in developed and developing countries. However, adoption rates in developing countries lag far behind. This paper draws on the Perceived eReadiness Model and research on the influence of inter-organizational relationships and economic-cultural contexts to explain the importance of three factorsâinter-organizational power dependence, cooperativeness, and regional economic-cultural differencesâfor achieving higher levels of Internet-based Electronic Data Interchange (EDI) in the developing country of China. We employ survey data to empirically test both the individual and joint influence of these factors. The findings suggest that beyond intra-organizational and external factors, managers and policy makers wanting to promote Internet-based EDI adoption in developing countries must also account for the inter-organizational relationships of firms and the economic and cultural circumstances of the regions in which they operate
Production and Decay of D_1(2420)^0 and D_2^*(2460)^0
We have investigated and final states and
observed the two established charmed mesons, the with mass
MeV/c and width MeV/c and
the with mass MeV/c and width
MeV/c. Properties of these final states, including
their decay angular distributions and spin-parity assignments, have been
studied. We identify these two mesons as the doublet predicted
by HQET. We also obtain constraints on {\footnotesize } as a function of the cosine of the relative phase of the two
amplitudes in the decay.Comment: 15 pages in REVTEX format. hardcopies with figures can be obtained by
sending mail to: [email protected]
Measurement of the branching fraction for
We have studied the leptonic decay of the resonance into tau
pairs using the CLEO II detector. A clean sample of tau pair events is
identified via events containing two charged particles where exactly one of the
particles is an identified electron. We find . The result is consistent with
expectations from lepton universality.Comment: 9 pages, RevTeX, two Postscript figures available upon request, CLNS
94/1297, CLEO 94-20 (submitted to Physics Letters B
Study of the B^0 Semileptonic Decay Spectrum at the Upsilon(4S) Resonance
We have made a first measurement of the lepton momentum spectrum in a sample
of events enriched in neutral B's through a partial reconstruction of B0 -->
D*- l+ nu. This spectrum, measured with 2.38 fb**-1 of data collected at the
Upsilon(4S) resonance by the CLEO II detector, is compared directly to the
inclusive lepton spectrum from all Upsilon(4S) events in the same data set.
These two spectra are consistent with having the same shape above 1.5 GeV/c.
From the two spectra and two other CLEO measurements, we obtain the B0 and B+
semileptonic branching fractions, b0 and b+, their ratio, and the production
ratio f+-/f00 of B+ and B0 pairs at the Upsilon(4S). We report b+/b0=0.950
(+0.117-0.080) +- 0.091, b0 = (10.78 +- 0.60 +- 0.69)%, and b+ = (10.25 +- 0.57
+- 0.65)%. b+/b0 is equivalent to the ratio of charged to neutral B lifetimes,
tau+/tau0.Comment: 14 page, postscript file also available at
http://w4.lns.cornell.edu/public/CLN
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