47,691 research outputs found

    Young stars at large distances from the galactic plane: mechanisms of formation

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    We have collected from the literature a list of early-type stars, situated at large distances from the galactic plane, for which evidence of youth seems convincing. We discuss two possible formation mechanisms for these stars: ejection from the plane by dynamical interactions within small clusters, and formation away from the plane, via induced shocks created by spiral density waves. We identify the stars that could be explained by each mechanism. We conclude that the ejection mechanism can account for about two thirds of the stars, while a combination of star formation at z = 500-800 pc from the plane and ejection, can account for 90 percent of these stars. Neither mechanism, nor both together, can explain the most extreme examples.Comment: 6 pages, No figures. Sixth Pacific Rim Conference on Stellar Astrophysics - A tribute to Helmut Abt, (Kluwer

    Estimates for the ergodic measure and polynomial stability of plane stochastic curve shortening flow

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    We establish moment estimates for the invariant measure of a stochastic partial differential equation describing motion by mean curvature flow in (1+1) dimension, leading to polynomial stability of the associated Markov semigroup. We also prove maximal dissipativity for the related Kolmogorov operator

    Deconvolution for an atomic distribution: rates of convergence

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    Let X1,...,XnX_1,..., X_n be i.i.d.\ copies of a random variable X=Y+Z,X=Y+Z, where Xi=Yi+Zi, X_i=Y_i+Z_i, and YiY_i and ZiZ_i are independent and have the same distribution as YY and Z,Z, respectively. Assume that the random variables YiY_i's are unobservable and that Y=AV,Y=AV, where AA and VV are independent, AA has a Bernoulli distribution with probability of success equal to 1−p1-p and VV has a distribution function FF with density f.f. Let the random variable ZZ have a known distribution with density k.k. Based on a sample X1,...,Xn,X_1,...,X_n, we consider the problem of nonparametric estimation of the density ff and the probability p.p. Our estimators of ff and pp are constructed via Fourier inversion and kernel smoothing. We derive their convergence rates over suitable functional classes. By establishing in a number of cases the lower bounds for estimation of ff and pp we show that our estimators are rate-optimal in these cases.Comment: 27 page

    In-situ thermally-reduced graphene oxide/epoxy composites: thermal and mechanical properties

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    Graphene has excellent mechanical, thermal, optical and electrical properties and this has made it a prime target for use as a filler material in the development of multifunctional polymeric composites. However, several challenges need to be overcome in order to take full advantage of the aforementioned properties of graphene. These include achieving good dispersion and interfacial properties between the graphene filler and the polymeric matrix. In the present work we report the thermal and mechanical properties of reduced graphene oxide/epoxy composites prepared via a facile, scalable and commercially-viable method. Electron micrographs of the composites demonstrate that the reduced graphene oxide (rGO) is well-dispersed throughout the composite. Although no improvements in glass transition temperature, tensile strength, and thermal stability in air of the composites were observed, good improvements in thermal conductivity (about 36%), tensile and storage moduli (more than 13%) were recorded with the addition of 2 wt% of rGO

    Doctor of Philosophy

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    dissertationComputer simulations of biomolecules can provide insight into biological structure and dynamics at the atomic level. For simulations to be accurate and reliable, the underlying force eld that describes that system has to tested and assessed against experimental values. Evaluating the latest AMBER nucleic acids force elds at microsecond time scales is important for determining how updated force eld parameter sets compare to earlier models and updated, competing models. The latest two improvements to the AMBER nucleic acid force eld were compared to each other and previous, widely used versions. Both of the latest versions, bsc1 and OL15, showed improvement over earlier versions and reproduced many structural properties in agreement with nuclear magnetic resonance (NMR) and X-ray crystallography experiments. Having a force eld that accurately models duplex DNA is important, but it is also necessary to validate protein-nucleic acid simulations. To examine this, the E2-DNA system was chosen for simulations to see if DNA backbone substates observed in the X-ray structure were reproducible in simulations. In particular, the BI/BII substates were scrutinized. The BI substate is dominant in duplex DNA but and dihedrals populate both trans/gauche- (t/g-) and gauche-/trans (g-/t) conformations, the latter being the BII state. It was determined that dinucleotide steps crystallized in the BII were correspondingly highly-populated in simulations. Additionally, and dihedrals were manipulated to decoy states and found to converge to native distributions on the microsecond time scale in E2-bound DNA, and in less time for free DNA. During the investigation of BII substates in E2-DNA, the surprising observation was made that BI/BII transitions are dominant modes of motion in E2-bound DNA. This inspired research into whether these modes are sequence-dependent or completely induced by the E2 protein, and if the dynamics are conserved across E2 types. Simulations of E2-DNA found that the BII state is determined by a combination of DNA sequence and E2 binding partner

    Relationship between infarct tissue characteristics and left ventricular remodeling in patients with versus without early revascularization for acute myocardial infarction as assessed with contrast-enhanced cardiovascular magnetic resonance imaging

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    Left ventricular (LV) remodeling following myocardial infarction (MI) is the result of complex interactions between various factors, including presence or absence of early revascularization. The impact of early revascularization on the relationship between infarct tissue characteristics and LV remodeling is incompletely known. Therefore, we investigated in patients with versus without successful early revascularization for acute MI potential relations between infarct tissue characteristics and LV remodeling with contrast-enhanced (CE) cardiovascular magnetic resonance (CMR). Patients with versus without successful early revascularization underwent CE-CMR for tissue characterization and assessment of LV remodeling including end-diastolic and end-systolic volumes, LV ejection fraction, and wall motion score index (WMSI). CE-CMR images were analyzed for infarct tissue characteristics including core-, peri- and total-infarct size, transmural extent, and regional scar scores. In early revascularized patients (n = 46), a larger area of infarct tissue correlated significantly with larger LV dimensions and a more reduced LV function (r = 0.39-0.68; all P ≤ 0.01). Multivariate analyses identified peri-infarct size as the best predictor of LV remodeling parameters (R2 = 0.44-0.62). In patients without successful early revascularization (n = 47), there was no correlation between infarct area and remodeling parameters; only peri-infarct size versus WMSI (r = 0.33; P = 0.03) and transmural extent versus LVEF (r = -0.27; P = 0.07) tended to be related. A correlation between infarct tissue characteristics and LV remodeling was found only in patients with early successful revascularization. Peri-infarct size was found to be the best determinant of LV remodeling. Our findings stress the importance of taking into account infarct tissue characteristics and success of revascularization when LV remodeling is studie
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