1,800 research outputs found
Flight test evaluation of an RAF high altitude partial pressure protective assembly
A partial pressure suit was evaluated during tests in an F-104 and F-15 as a protective garment for emergency descents. The garment is an pressure jerkin and modified anti-g suit combined with an oronasal mask. The garment can be donned and doffed at the aircraft to minimize thermal buildup. The oronasal mask was favored by the pilots due to its immobility on the face during high g-loading. The garment was chosen to provide optimum dexterity for the pilot, which is not available in a full pressure suit, while protecting the pilot at altitudes up to 18,288 meters, during a cabin decompression, and subsequent aircraft descent. During cabin decompressions in the F-104 and F-15, cabin pressure altitude was measured at various aircraft angles of attack, Mach numbers, and altitudes to determine the effect of the aerodynamic slipstream on the cabin altitude
The Compact Central Object in Cas A: A Neutron Star with Hot Polar Caps or a Black Hole?
The central pointlike X-ray source of the Cas A supernova remnant was
discovered in the Chandra First Light Observation and found later in the
archival ROSAT and Einstein images. The analysis of these data does not show
statistically significant variability of the source. The power-law fit yields
the photon index 2.6-4.1, and luminosity (2-60)e34 erg/s, for d=3.4 kpc. The
power-law index is higher, and the luminosity lower, than those observed
fromvery young pulsars. One can fit the spectrum equally well with a blackbody
model with T=6-8 MK, R=0.2-0.5 km, L=(1.4-1.9)e33 erg/s. The inferred radii are
too small, and the temperatures too high, for the radiationcould be interpreted
as emitted from the whole surface of a uniformly heated neutron star. Fits with
the neutron star atmosphere models increase the radius and reduce the
temperature, but these parameters are still substantially different from those
expected for a young neutron star. One cannot exclude, however, that the
observed emission originates from hot spots on a cooler neutron star surface.
Because of strong interstellar absorption, the possible low-temperature
component gives a small contribution to the observed spectrum; an upper limit
on the (gravitationally redshifted) surface temperature is < 1.9-2.3 MK.
Amongst several possible interpretations, we favor a model of a strongly
magnetized neutron star with magnetically confined hydrogen or helium polar
caps on a cooler iron surface. Alternatively, the observed radiation may be
interpreted as emitted by a compact object (more likely, a black hole)
accreting from a fossil disk or from a late-type dwarf in a close binary.Comment: 12 pages, 2 figures, submitted to ApJ
The X-ray Source at the Center of the Cassiopeia A Supernova Remnant
We present the first results of an XMM-Newton observation of the central
X-ray source in the Cas A supernova remnant. The spectrum can be fit equally
well with an absorbed steep power law (alpha~3, N_H~1.5x10^22 cm^-2) or with a
bremsstrahlung with temperature kT~2.4 keV and N_H~10^22 cm^-2. A blackbody
model (kT~0.7 keV) gives a slightly worse fit and requires a column density
N_H~5x10^21 cm^-2 and an emitting area with radius ~0.3 km (for d=3.4 kpc). A
search for pulsations for periods longer than 150 ms gave negative results. The
3 sigma upper limits on the pulsed fraction are ~13% for P>0.3 s and ~7% for
P>3 s. The overall properties of the central X-ray source in Cas A are
difficult to explain in terms of a rapidly spinning neutron star with a
canonical magnetic field of ~10^12 G, and are more similar to those of slowly
rotating neutron stars such as the Anomalous X-ray Pulsars.Comment: 15 pages, latex, 3 figures, to appear in The Astrophysical Journal;
Revised version with more details on spectral analysis, fig. 1 and 2 slightly
changed, revised flux value
Search for an Near-IR Counterpart to the Cas A X-ray Point Source
We report deep near-infrared and optical observations of the X-ray point
source in the Cassiopeia A supernova remnant, CXO J232327.9+584842. We have
identified a J=21.4 +/- 0.3 mag and Ks=20.5 +/- 0.3 mag source within the
1-sigma error circle, but we believe this source is a foreground Pop II star
with Teff=2600-2800 K at a distance of ~2 kpc, which could not be the X-ray
point source. We do not detect any sources in this direction at the distance of
Cas A, and therefore place 3-sigma limits of R >~ 25 mag, F675W >~ 27.3 mag, J
>~ 22.5 mag and Ks >~ 21.2 mag (and roughly H >~ 20 mag) on emission from the
X-ray point source, corresponding to M_{R} >~ 8.2 mag, M_{F675W} >~ 10.7 mag,
M_{J} >~ 8.5 mag, M_{H} >~ 6.5 mag, and M_{Ks} >~ 8.0 mag, assuming a distance
of 3.4 kpc and an extinction A_{V}=5 mag.Comment: 14 pages, 7 figures. Accepted by Ap
Analysis and characterization of differential gene expression during rapid trophoblastic elongation in the pig using suppression subtractive hybridization
During late peri-implantation development, porcine conceptuses undergo a rapid (2â3 hrs) morphological transformation from a 10 mm sphere to a thin filamentous form greater than 150 mm in length. Elongation of the conceptus is important for establishing adequate placental surface area needed for embryo and fetal survival throughout gestation. Genes involved with triggering this unique transition in conceptus development are not well defined. Objective of the present study was to utilize suppression subtractive hybridization (SSH) to characterize the change in gene expression during conceptus transformation from spherical (8â9 mm) to tubular (15â40 mm) to early filamentous (>150 mm) morphology. Spherical, tubular, and filamentous conceptuses were collected from pregnant gilts and subjected to SSH. Forward and reverse subtractions were performed to identify candidate genes differentially expressed during spherical to tubular and tubular to filamentous transition. A total of 384 transcripts were differentially screened to ensure unique expression. Of the transcripts screened, sequences were obtained for 142 that were confirmed to be differentially expressed among the various morphologies. Gene expression profiles during rapid trophoblastic elongation were generated for selected mRNAs using quantitative real-time PCR. During the transition from tubular to early filamentous conceptuses, s-adenosylhomocysteine hydrolase and heat shock cognate 70 kDa expression were significantly enhanced. A novel unknown gene was isolated and shown to be significantly up-regulated at the onset of rapid trophoblastic elongation and further enhanced in filamentous conceptuses
Factors affecting metal mobilisation during oxidation of sulphidic, sandy wetland substrates
Most metals accumulate as sulphides under anoxic conditions in wetland substrates, reducing their bioavailability due to the solubility of metal sulphides. However, upon oxidation of these sulphides when the substrate is occasionally oxidised, metals can be released from the solid phase to the pore water or overlaying surface water. This release can be affected by the presence of carbonates, organic matter and clay. We compared changes of Cd, Cu and Zn mobility (CaCl2 extraction) during oxidation of a carbonate-rich and a carbonate-poor sulphidic, sandy wetland substrate. In addition, we studied how clay with low and high cation sorption capacity (bentonite and kaolinite, respectively) and organic matter (peat) can counteract Cd, Cu and Zn release during oxidation of both carbonate-rich and carbonate-poor sulphidic sediments. CaCl2-extractability of Cu, a measure for its availability, is low in both carbonate-poor and carbonate-rich substrates, whereas its variability is high. The availability of Cd and Zn is much higher and increases when peat is supplied to carbonate-poor substrates. A strong reduction of Cd and Zn extractability is observed when clay is added to carbonate-poor substrates. This reduction depends on the clay type. Most observations could be explained taking into account pH differences between treatments, with kaolinite resulting in a lower pH in comparison to bentonite. These pH differences affect the presence and characteristics of dissolved organic carbon and the metal speciation, which in turns affects the interaction of metals with the solid soil phase. In carbonate-rich substrates, Cd and Zn availability is lower and the effects of peat and clay amendment are less clear. The latter can also be attributed to the high pH and lack of pH differences between treatments
Upper Limits On Periodic, Pulsed Radio Emission from the X-Ray Point Source in Cassiopeia A
The Chandra X-ray Observatory recently discovered an X-ray point source near
the center of Cassiopeia A, the youngest known Galactic supernova remnant. We
have conducted a sensitive search for radio pulsations from this source with
the Very Large Array, taking advantage of the high angular resolution of the
array to resolve out the emission from the remnant itself. No convincing
signatures of a dispersed, periodic source or of isolated dispersed pulses were
found, whether for an isolated or a binary source. We derive upper limits of 30
and 1.3 mJy at 327 and 1435 MHz for the phase-averaged pulsed flux density from
this source. The corresponding luminosity limits are lower than those for any
pulsar with age less than 10^4 years. The sensitivities of our search to single
pulses were 25 and 1.0 Jy at 327 and 1435 MHz. For comparison, the Crab pulsar
emits roughly 80 pulses per minute with flux densities greater than 100 Jy at
327 MHz and 8 pulses per minute with flux densities greater than 50 Jy at 1435
MHz. These limits are consistent with the suggestion that the X-ray point
source in Cas A adds to the growing number of neutron stars which are not radio
pulsars.Comment: accepted by ApJ Letter
Toward a simulation approach for alkene ring-closing metathesis : scope and limitations of a model for RCM
A published model for revealing solvent effects on the ring-closing metathesis (RCM) reaction of di-Et diallylmalonate 7 has been evaluated over a wider range of conditions, to assess its suitability for new applications. Unfortunately, the model is too flexible and the published rate consts. do not agree with exptl. studies in the literature. However, by fixing the values of important rate consts. and restricting the concn. ranges studied, useful conclusions can be drawn about the relative rates of RCM of different substrates, precatalyst concn. can be simulated accurately and the effect of precatalyst loading can be anticipated. Progress has also been made toward applying the model to precatalyst evaluation, but further modifications to the model are necessary to achieve much broader aims
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Thorium Energy Futures
The potential for thorium as an alternative or supplement to uranium in fission power generation has long been recognised, and several reactors, of various types, have already operated using thorium-based fuels. Accelerator Driven Subcritical (ADS) systems have benefits and drawbacks when compared to conventional critical thorium reactors, for both solid and molten salt fuels. None of the four options â liquid or solid, with or without an accelerator â can yet be rated as better or worse than the other three, given today's knowledge. We outline the research that will be necessary to lead to an informed choice
The business of cultural heritage tourism: critical success factors
This paper explores critical success factors (CSFs) required for cultural heritage tourism (CHT) operation and how these relate to commercial focus. The literature indicates tension between conservation of authenticity and commercial focus as it is seen to undermine authenticity, potentially degrading its quality and ultimate success as a tourism product. A list of nine key CHT business success factors was devised based on the published literature. Managers and operators of a range of Australian CHT operations were interviewed regarding achievement of CSFs. The operations were broadly categorised according to the level of commercial focus. The level of commercial focus was cross tabulated with the number of CHT business CSFs achieved. While all places in this study had addressed authenticity, CHT places presenting highly commercialised products tended to meet the criteria for achieving a greater number of CSFs than their less commercialised counter-parts. This has implications for sustainable CHT operation practices
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