Detection of a z=0.0515, 0.0522 absorption system in the QSO S4 0248+430 due to an intervening galaxy

In some of the few cases where the line of sight to a Quasi-Stellar Object (QSO) passes near a galaxy, the galaxy redshift is almost identical to an absorption redshift in the spectrum of the QSO. Although these relatively low redshift QSO-galaxy pairs may not be typical of the majority of the narrow heavy-element QSO absorption systems, they provide a direct measure of column densities in the outer parts of galaxies and some limits on the relative abundances of the gas. Observations are presented here of the QSO S4 0248+430 and a nearby anonymous galaxy (Kuhr 1977). The 14 second separation of the line of sight to the QSO (z sub e = 1.316) and the z=0.052 spiral galaxy, (a projected separation of 20 kpc ((h sub o = 50, q sub o = 0)), makes this a particularly suitable pair for probing the extent and content of gas in the galaxy. Low resolution (6A full width half maximum), long slit charge coupled device (CCD) spectra show strong CA II H and K lines in absorption at the redshift of the galaxy (Junkkarinen 1987). Higher resolution spectra showing both Ca II H and K and Na I D1 and D2 in absorption and direct images are reported here

Massively parallel I/O: Building an infrastructure for parallel computing

The solution of Grand Challenge Problems will require computations that are too large to fit in the memories of even the largest machines. Inevitably, new designs of I/O systems will be necessary to support them. This report describes the work in investigating I/O subsystems for massively parallel computers. Specifically, the authors investigated out-of-core algorithms for common scientific calculations present several theoretical results. They also describe several approaches to parallel I/O, including partitioned secondary storage and choreographed I/O, and the implications of each to massively parallel computing

Temperature and Kinematics of CIV Absorption Systems

We use Keck HIRES spectra of three intermediate redshift QSOs to study the physical state and kinematics of the individual components of CIV selected heavy element absorption systems. Fewer than 8 % of all CIV lines with column densities greater than 10^{12.5} cm^{-2} have Doppler parameters b < 6 km/s. A formal decomposition into thermal and non-thermal motion using the simultaneous presence of SiIV gives a mean thermal Doppler parameter b_{therm}(CIV) = 7.2 km/s, corresponding to a temperature of 38,000 K although temperatures possibly in excess of 300,000 K occur occasionally. We also find tentative evidence for a mild increase of temperature with HI column density. Non-thermal motions within components are typically small (< 10 km/s) for most systems, indicative of a quiescent environment. The two-point correlation function (TPCF) of CIV systems on scales up to 500 km/s suggests that there is more than one source of velocity dispersion. The shape of the TPCF can be understood if the CIV systems are caused by ensembles of objects with the kinematics of dwarf galaxies on a small scale, while following the Hubble flow on a larger scale. Individual high redshift CIV components may be the building blocks of future normal galaxies in a hierarchical structure formation scenario.Comment: submitted to the ApJ Letters, March 16, 1996 (in press); (13 Latex pages, 4 Postscript figures, and psfig.sty included

The mapping class group and the Meyer function for plane curves

For each d>=2, the mapping class group for plane curves of degree d will be defined and it is proved that there exists uniquely the Meyer function on this group. In the case of d=4, using our Meyer function, we can define the local signature for 4-dimensional fiber spaces whose general fibers are non-hyperelliptic compact Riemann surfaces of genus 3. Some computations of our local signature will be given.Comment: 24 pages, typo adde

Muscarinic modulation of conductances underlying the afterhyperpolarization in neurons of the rat basolateral amygdala

The excitability level of pyramidal neurons in the basolateral amygdala (BLA) is greatly increased following muscarinic receptor activation, an effect associated with an increased rate of action potential firing and reduction of the afterhyperpolarization (AHP). We impaled BLA pyramidal neurons in slices of rat ventral forebrain with a single microelectrode to examine the currents underlying the AHP and spike frequency accomodation and determine their sensitivities to muscarinic modulation. In voltage-clamp, depolarizing steps were followed by biphasic outward tail currents, consisting of rapidly decaying (IFast) and slowly decaying (ISlow) current components. These corresponded temporally with the medium and slow portions of the AHP, respectively. The reversal potential or the IFast component of the AHP tail current shifted in the depolarizing direction with increases in the extracellular K+ concentration. The amplitude of IFast was reduced during perfusion of 0-Ca2+ medium or by superfusion of TEA (1-5 mM) or carbachol (10-40 [mu]M). It is suggested that IFast was produced by the rapidly decaying Ca2+-activated K+ current (IC) and the muscarinic-sensitive M-current (IM). The ISlow tail current component reversed at the estimated values for EK in medium containing either normal or elevated K+ levels. This component was eliminated by perfusion of 0-Ca2+ medium or inclusion of cyclic-AMP in the recording electrode. It was not blocked by TEA (5 mM) or apamin (50-500 nM), but was reduced by carbachol in a dose-dependent manner (IC50=0.5 [mu]M). Electrical stimulation cholinergic afferent pathways to the BLA produced inhibition of ISlow, an effect which was enhanced by eserine and prevented by atropine. Loss of the ISlow component was always accompanied by similar reductions in accomodation and the slow AHP. It was concluded that this tail current component resulted from the slowly decaying Ca2+-activated K+ current, IAHP. Thus, the muscarinic inhibition of IAHP contributes to the enhanced excitability exhibited by BLA pyramidal neurons following cholinergic stimulation.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/30577/1/0000212.pd

3D seismic imaging on massively parallel computers

The ability to image complex geologies such as salt domes in the Gulf of Mexico and thrusts in mountainous regions is a key to reducing the risk and cost associated with oil and gas exploration. Imaging these structures, however, is computationally expensive. Datasets can be terabytes in size, and the processing time required for the multiple iterations needed to produce a velocity model can take months, even with the massively parallel computers available today. Some algorithms, such as 3D, finite-difference, prestack, depth migration remain beyond the capacity of production seismic processing. Massively parallel processors (MPPs) and algorithms research are the tools that will enable this project to provide new seismic processing capabilities to the oil and gas industry. The goals of this work are to (1) develop finite-difference algorithms for 3D, prestack, depth migration; (2) develop efficient computational approaches for seismic imaging and for processing terabyte datasets on massively parallel computers; and (3) develop a modular, portable, seismic imaging code

In-situ radiation measurements of the C1 and C2 waste storage tank vault

In August of 1996, the Applied Radiation Measurements Department (ARMD) of the Waste Management and Remedial Action Division (WMRAD) at Oak Ridge National Laboratory (ORNL) was tasked with characterizing the radiation fields in the C{sub 1} and C{sub 2} Liquid Low Level Waste (LLLW) tank vault located at ORNL. These in-situ measurements were made to provide data for evaluating the potential radiological conditions for personnel working in or around the vault during future planned activities. This report describes the locations where measurements were made, the types of radiation detection instruments used, the methods employed, the problems encountered and resolved, and discusses the results obtained

Multiple effects of long-term morphine treatment on postsynaptic [beta]-adrenergic receptor function in hippocampus: an intracellular analysis

We previously reported that [beta]-adrenergic receptors are increased in cerebral cortex and hippocampus in rats treated chronically with morphine and subsequently down-regulated after morphine withdrawal [22,23]. The changes in receptor density in hippocampus were accompanied by a corresponding super- and subsensitivity, respectively, in [beta]-adrenergic responsiveness, as assessed electrophysiologically by measuring the ability of isoproterenol to augment population spike responses in the slice. In this study, we compared the ability of isoproterenol to reduce the Ca2+-activated K+ slow afterhyperpolarization (slow AHP) in pyramidal neurons in hippocampal slices from opiate-naive and chronic morphine-treated rats to determine whether such changes in [beta]-adrenergic receptor function are localized postsynaptically. Chronic treatment of rats with morphine produced a 3.5-fold parallel shift to the left in the concentration-response curve for isoproterenol and reduced the EC50 from 4.8 +/- 1.3 to 1.4 +/- 0.5 nM. In contrast, sensitivity and maximal responsiveness to isoproterenol was markedly decreased in pyramidal neurons recorded in slices from morphine withdrawn animals. The concentration-response curves for inhibition of the slow AHP by carbachol or forskolin were not affected by chronic morphine treatment. However, blockade of the slow AHP by forskolin was significantly reduced in pyramidal neurons studied after morphine withdrawal. These data suggest that the increase in electrophysiological responsiveness to [beta]-adrenergic receptor stimulation found in hippocampus after chronic morphine treatment most likely resulted from an up-regulation in postsynaptic membrane receptors, whereas alterations occurring beyond the receptor level may be involved in the desentization that is associated with morphine withdrawal.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/31332/1/0000241.pd

Simulations of hydrodynamic interactions among immersed particles in stokes flow using a massively parallel computer

In this paper, a massively parallel implementation of the boundary element method to study particle transport in Stokes flow is discussed. The numerical algorithm couples the quasistatic Stokes equations for the fluid with kinematic and equilibrium equations for the particles. The formation and assembly of the discretized boundary element equations is based on the torus-wrap mapping as opposed to the more traditional row- or column-wrap mappings. The equation set is solved using a block Jacobi iteration method. Results are shown for an example application problem, which requires solving a dense system of 6240 equations more than 1200 times