2,269 research outputs found

    Complex circular subsidence structures in tephra deposited on large blocks of ice: Varða tuff cone, Öræfajökull, Iceland

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    Several broadly circular structures up to 16 m in diameter, into which higher strata have sagged and locally collapsed, are present in a tephra outcrop on southwest Öræfajökull, southern Iceland. The tephra was sourced in a nearby basaltic tuff cone at Varða. The structures have not previously been described in tuff cones, and they probably formed by the melting out of large buried blocks of ice emplaced during a preceding jökulhlaup that may have been triggered by a subglacial eruption within the Öræfajökull ice cap. They are named ice-melt subsidence structures, and they are analogous to kettle holes that are commonly found in proglacial sandurs and some lahars sourced in ice-clad volcanoes. The internal structure is better exposed in the Varða examples because of an absence of fluvial infilling and reworking, and erosion of the outcrop to reveal the deeper geometry. The ice-melt subsidence structures at Varða are a proxy for buried ice. They are the only known evidence for a subglacial eruption and associated jökulhlaup that created the ice blocks. The recognition of such structures elsewhere will be useful in reconstructing more complete regional volcanic histories as well as for identifying ice-proximal settings during palaeoenvironmental investigations

    The Globular Cluster System of M60 (NGC 4649). I. CFHT MOS Spectroscopy and Database

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    We present the measurement of radial velocities for globular clusters in M60, giant elliptical galaxy in the Virgo cluster. Target globular cluster candidates were selected using the Washington photometry based on the deep 16\arcmin \times 16\arcmin images taken at the KPNO 4m and using the VIVI photometry derived from the HST/WFPC2 archive images. The spectra of the target objects were obtained using the Multi-Object Spectrograph (MOS) at the Canada-France-Hawaii Telescope (CFHT). We have measured the radial velocity for 111 objects in the field of M60: 93 globular clusters (72 blue globular clusters with 1.0(CT1)<1.71.0\le(C-T_1)<1.7 and 21 red globular clusters with 1.7(CT1)<2.41.7\le(C-T_1)<2.4), 11 foreground stars, 6 small galaxies, and the nucleus of M60. The measured velocities of the 93 globular clusters range from 500\sim 500 km s1^{-1} to 1600\sim 1600 km s1^{-1}, with a mean value of 107025+271070_{-25}^{+27} km s1^{-1}, which is in good agreement with the velocity of the nucleus of M60 (vgal=1056v_{\rm gal}=1056 km s1^{-1}). Combining our results with data in the literature, we present a master catalog of radial velocities for 121 globular clusters in M60. The velocity dispersion of the globular clusters in the master catalog is found to be 23414+13234_{-14}^{+13} km s1^{-1} for the entire sample, 22316+13223_{-16}^{+13} km s1^{-1} for 83 blue globular clusters, and 25831+21258_{-31}^{+21} km s1^{-1} for 38 red globular clusters.Comment: 29 pages, 8 figures. To appear in Ap

    Notes on Supersymmetry Enhancement of ABJM Theory

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    We study the supersymmetry enhancement of ABJM theory. Starting from a N=2{\cal N}=2 supersymmetric Chern-Simons matter theory with gauge group U(2)×\timesU(2) which is a truncated version of the ABJM theory, we find by using the monopole operator that there is additional N=2{\cal N}=2 supersymmetry related to the gauge group. We show this additional supersymmetry can combine with N=6{\cal N}=6 supersymmetry of the original ABJM theory to an enhanced N=8{\cal N}=8 SUSY with gauge group U(2)×\timesU(2) in the case k=1,2k=1,2. We also discuss the supersymmetry enhancement of the ABJM theory with U(NN)×\timesU(NN) gauge group and find a condition which should be satisfied by the monopole operator.Comment: 23 pages, no figure, minor corrections, version to appear in JHE

    Orientational pinning and transverse voltage: Simulations and experiments in square Josephson junction arrays

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    We study the dependence of the transport properties of square Josephson Junctions arrays with the direction of the applied dc current, both experimentally and numerically. We present computational simulations of current-voltage curves at finite temperatures for a single vortex in the array (Ha2/Φ0=f=1/L2Ha^2/\Phi_0=f=1/L^2), and experimental measurements in 100×1000100\times1000 arrays under a low magnetic field corresponding to f0.02f\approx0.02. We find that the transverse voltage vanishes only in the directions of maximum symmetry of the square lattice: the [10] and [01] direction (parallel bias) and the [11] direction (diagonal bias). For orientations different than the symmetry directions, we find a finite transverse voltage which depends strongly on the angle ϕ\phi of the current. We find that vortex motion is pinned in the [10] direction (ϕ=0\phi=0), meaning that the voltage response is insensitive to small changes in the orientation of the current near ϕ=0\phi=0. We call this phenomenon orientational pinning. This leads to a finite transverse critical current for a bias at ϕ=0\phi=0 and to a transverse voltage for a bias at ϕ0\phi\not=0. On the other hand, for diagonal bias in the [11] direction the behavior is highly unstable against small variations of ϕ\phi, leading to a rapid change from zero transverse voltage to a large transverse voltage within a few degrees. This last behavior is in good agreement with our measurements in arrays with a quasi-diagonal current drive.Comment: 9 pages, 9 figure

    GALEX UV Color-Magnitude Relations and Evidence for Recent Star Formation in Early-type Galaxies

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    We have used the GALEX UV photometric data to construct a first near-ultraviolet (NUV) color-magnitude relation (CMR) for the galaxies pre-classified as early-type by SDSS studies. The NUV CMR is a powerful tool for tracking the recent star formation history in early-type galaxies, owing to its high sensitivity to the presence of young stellar populations. Our NUV CMR for UV-weak galaxies shows a well-defined slope and thus will be useful for interpreting the restframe NUV data of distant galaxies and studying their star formation history. Compared to optical CMRs, the NUV CMR shows a substantially larger scatter, which we interpret as evidence of recent star formation activities. Roughly 15% of the recent epoch (z < 0.13) bright (M[r] < -22) early-type galaxies show a sign of recent (< 1Gyr) star formation at the 1-2% level (lower limit) in mass compared to the total stellar mass. This implies that low level residual star formation was common during the last few billion years even in bright early-type galaxies.Comment: This paper will be published as part of the Galaxy Evolution Explorer (GALEX) Astrophysical Journal Letters Special Issue. Links to the full set of papers will be available at http://www.galex.caltech.edu/PUBLICATIONS/ after November 22, 200

    PCA-based lung motion model

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    Organ motion induced by respiration may cause clinically significant targeting errors and greatly degrade the effectiveness of conformal radiotherapy. It is therefore crucial to be able to model respiratory motion accurately. A recently proposed lung motion model based on principal component analysis (PCA) has been shown to be promising on a few patients. However, there is still a need to understand the underlying reason why it works. In this paper, we present a much deeper and detailed analysis of the PCA-based lung motion model. We provide the theoretical justification of the effectiveness of PCA in modeling lung motion. We also prove that under certain conditions, the PCA motion model is equivalent to 5D motion model, which is based on physiology and anatomy of the lung. The modeling power of PCA model was tested on clinical data and the average 3D error was found to be below 1 mm.Comment: 4 pages, 1 figure. submitted to International Conference on the use of Computers in Radiation Therapy 201

    Malaria-associated atypical memory B cells exhibit markedly reduced B cell receptor signaling and effector function

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    Protective antibodies in Plasmodium falciparum malaria are only acquired after years of repeated infections. Chronic malaria exposure is associated with a large increase in atypical memory B cells (MBCs) that resemble B cells expanded in a variety of persistent viral infections. Understanding the function of atypical MBCs and their relationship to classical MBCs will be critical to developing effective vaccines for malaria and other chronic infections. We show that VH gene repertoires and somatic hypermutation rates of atypical and classical MBCs are indistinguishable indicating a common developmental history. Atypical MBCs express an array of inhibitory receptors and B cell receptor (BCR) signaling is stunted in atypical MBCs resulting in impaired B cell responses including proliferation, cytokine production and antibody secretion. Thus, in response to chronic malaria exposure, atypical MBCs appear to differentiate from classical MBCs becoming refractory to BCR-mediated activation and potentially interfering with the acquisition of malaria immunity. DOI: http://dx.doi.org/10.7554/eLife.07218.00

    Enhanced Supersymmetry of Nonrelativistic ABJM Theory

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    We study the supersymmetry enhancement of nonrelativistic limits of the ABJM theory for Chern-Simons level k=1,2k=1,2. The special attention is paid to the nonrelativistic limit (known as `PAAP' case) containing both particles and antiparticles. Using supersymmetry transformations generated by the monopole operators, we find additional 2 kinematical, 2 dynamical, and 2 conformal supercharges for this case. Combining with the original 8 kinematical supercharges, the total number of supercharges becomes maximal: 14 supercharges, like in the well-known PPPP limit. We obtain the corresponding super Schr\"odinger algebra which appears to be isomorphic to the one of the PPPP case. We also discuss the role of monopole operators in supersymmetry enhancement and partial breaking of supersymmetry in nonrelativistic limit of the ABJM theory.Comment: 22 pages, references added, version to appear in JHE

    Estimated Risk of HIV Acquisition and Practice for Preventing Occupational Exposure: A Study of Healthcare Workers at Tumbi and Dodoma Hospitals, Tanzania.

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    Health care workers (HCWs) are at risk of acquiring human immuno-deficiency virus (HIV) and other infections via exposure to infectious patients' blood and body fluids. The main objective of this study was to estimate the risk of HIV transmission and examine the practices for preventing occupational exposures among HCWs at Tumbi and Dodoma Hospitals in Tanzania. This study was carried out in two hospitals, namely, Tumbi in Coast Region and Dodoma in Dodoma Region. In each facility, hospital records of occupational exposure to HIV infection and its management were reviewed. In addition, practices to prevent occupational exposure to HIV infection among HCWs were observed. The estimated risk of HIV transmission due to needle stick injuries was calculated to be 7 cases per 1,000,000 HCWs-years. Over half of the observed hospital departments did not have guidelines for prevention and management of occupational exposure to HIV infections and lacked well displayed health and safety instructions. Approximately, one-fifth of the hospital departments visited failed to adhere to the instructions pertaining to correlation between waste materials and the corresponding colour coded bag/container/safety box. Seventy four percent of the hospital departments observed did not display instructions for handling infectious materials. Inappropriate use of gloves, lack of health and safety instructions, and lack of use of eye protective glasses were more frequently observed at Dodoma Hospital than at Tumbi Hospital. The poor quality of the hospital records at the two hospitals hampered our effort to characterise the risk of HIV infection acquisition by HCWs. Greater data completeness in hospital records is needed to allow the determination of the actual risk of HIV transmission for HCWs. To further reduce the risk of HIV infection due to occupational exposure, hospitals should be equipped with sufficient personal protective equipment (PPE) and HCWs should be reminded of the importance of adhering to universal precautions

    Search for CP Violation in the Decays D0KS0P0D^0\rightarrow K^0_S P^0

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    We have searched for CP violation in the decays D0KS0P0D^0\rightarrow K^0_S P^0 where P0P^0 denotes a neutral pseudo-scalar meson which is either a π0\pi^0, η\eta, or η\eta' using KEKB asymmetric-energy e+ee^+e^- collision data corresponding to an integrated luminosity of 791 fb1^{-1} collected with the Belle detector. No evidence of significant CP violation is observed. We report the most precise CP asymmetry measurement in the decay D0KS0π0D^0\rightarrow K^0_S\pi^0 to date: ACPD0KS0π0=(0.28±0.19±0.10)A_{CP}^{D^0\rightarrow K^0_S\pi^0}=(-0.28\pm0.19\pm0.10)%. We also report the first measurements of CP asymmetries in the decays D0KS0ηD^0\rightarrow K^0_S\eta and D0KS0ηD^0\rightarrow K^0_S\eta': ACPD0KS0η=(+0.54±0.51±0.16)A_{CP}^{D^0\rightarrow K^0_S\eta}=(+0.54\pm0.51\pm0.16)% and ACPD0KS0η=(+0.98±0.67±0.14)A_{CP}^{D^0\rightarrow K^0_S\eta'}=(+0.98\pm0.67\pm0.14)%, respectively
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