31,359 research outputs found

    Modeling the chemical evolution of Omega Centauri using three-dimensional hydrodynamical simulations

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    We present a hydrodynamical and chemical model for the globular cluster Omega Cen, under the assumption that it is the remnant of an ancient dwarf spheroidal galaxy (dSph), the bulk of which was disrupted and accreted by our Galaxy ~10 Gyr ago. We highlight the very different roles played by Type II and Type Ia supernovae (SNe) in the chemical enrichment of the inner regions of the putative parent dSph. While the SNe II pollute the interstellar medium rather uniformly, the SNe Ia ejecta may remain confined inside dense pockets of gas as long as succesive SNe II explosions spread them out. Stars forming in such pockets have lower alpha-to-iron ratios than the stars forming elsewhere. Owing to the inhomogeneous pollution by SNe Ia, the metal distribution of the stars in the central region differs substantially from that of the main population of the dwarf galaxy, and resembles that observed in Omega Cen. This inhomogeneous mixing is also responsible for a radial segregation of iron-rich stars with depleted [alpha/Fe] ratios, as observed in some dSphs. Assuming a star formation history of ~1.5 Gyr, our model succeeds in reproducing both the iron and calcium distributions observed in Omega Cen and the main features observed in the empirical alpha/Fe versus Fe/H plane. Finally, our model reproduces the overall spread of the color-magnitude diagram, but fails in reproducing the morphology of the SGB-a and the double morphology of the main sequence. However, the inhomogeneous pollution reduces (but does not eliminate) the need for a significantly enhanced helium abundance to explain the anomalous position of the blue main sequence. Further models taking into account the dynamical interaction of the parent dwarf galaxy with the Milky Way and the effect of AGB pollution will be required.Comment: 15 pages, 13 figures. MNRAS accepte

    Three-body structure of the nnΛnn\Lambda system with ΛN−ΣN\Lambda N-\Sigma N coupling

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    The structure of the three-body nnΛnn\Lambda system, which has been observed recently by the HypHI collaboration, is investigated taking ΛN−ΣN\Lambda N-\Sigma N coupling explicitly into account. The YNYN and NNNN interactions employed in this work reproduce the binding energies of Λ3^3_{\Lambda}H, Λ4^4_{\Lambda}H and Λ4^4_{\Lambda}He. We do not find any Λ3n^3_{\Lambda}n bound state, which contradicts the interpretation of the data reported by the HypHI collaboration.Comment: To be publsihed in PRC as a Rapid communicatio

    Two-dimensional oscillating airfoil test apparatus

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    A two dimensional oscillating airfoil test apparatus is presented as a method of measuring unsteady aerodynamic forces on an airfoil or rotor blade section. The oscillating airfoil test rig, which is being built for use in an 11 X 11-foot transonic wind tunnel (speed range M = 0.4 - 1.4), will allow determination of unsteady loadings and detailed pressure distributions on representative airfoil sections undergoing simulated pitching and flapping motions. The design details of the motion generating system and supporting structure are presented. This apparatus is now in the construction phase

    Three-nucleon interactions: A frontier in nuclear structure

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    Three-nucleon interactions are a frontier in understanding and predicting the structure of strongly-interacting matter in laboratory nuclei and in the cosmos. We present results and discuss the status of first calculations with microscopic three-nucleon interactions beyond light nuclei. This coherent effort is possible due to advances based on effective field theory and renormalization group methods in nuclear physics.Comment: 7 pages, 11 figures, talk at International Symposium on New Facet of Three-Nucleon Force (FM50), Tokyo, October, 200

    Importance of Baryon-Baryon Coupling in Hypernuclei

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    The ΛN−ΣN\Lambda N - \Sigma N coupling in Λ\Lambda--hypernuclei and ΛΛ−ΞN\Lambda \Lambda - \Xi N coupling in ΛΛ\Lambda \Lambda--hypernuclei produce novel physics not observed in the conventional, nonstrange sector. Effects of Λ↔Σ\Lambda \leftrightarrow \Sigma conversion in Λ3^3_{\Lambda}H are reviewed. The role of ΛN−ΣN\Lambda N - \Sigma N coupling suppression in the A=4,5A=4,5 Λ\Lambda--hypernuclei due to Pauli blocking is highlighted, and the implications for the structure of    Λ10^{10}_{\;\, \Lambda}B are explored. Suppression of ΛΛ−ΞN\Lambda \Lambda - \Xi N conversion in ΛΛ     6^{\;\;\, 6}_{\Lambda \Lambda}He is hypothesized as the reason that the matrix element is small. Measurement of ΛΛ     4^{\;\;\, 4}_{\Lambda \Lambda}H is proposed to investigate the full ΛΛ−ΞN\Lambda \Lambda - \Xi N interaction. The implication for ΛΛ\Lambda \Lambda analog states is discussed.Comment: 17 pages LATEX, 1 figure uuencoded postscrip

    On Dwarf Galaxies as the Source of Intracluster Gas

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    Recent observational evidence for steep dwarf galaxy luminosity functions in several rich clusters has led to speculation that their precursors may be the source of the majority of gas and metals inferred from intracluster medium (ICM) x-ray observations. Their deposition into the ICM is presumed to occur through early supernovae-driven winds, the resultant systems reflecting the photometric and chemical properties of the low luminosity dwarf spheroidals and ellipticals we observe locally. We consider this scenario, utilising a self-consistent model for spheroidal photo-chemical evolution and gas ejection via galactic superwinds. Insisting that post-wind dwarfs obey the observed colour-luminosity-metallicity relations, we conclude that the bulk of the ICM gas and metals does not originate within their precursors.Comment: 43 pages, 8 figures, LaTeX, also available at http://msowww.anu.edu.au/~gibson/publications.html, to appear in ApJ, Vol 473, 1997, in pres

    System maintenance manual for master modeling of aerodynamic surfaces by three-dimensional explicit representation

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    A system of computer programs has been developed to model general three-dimensional surfaces. Surfaces are modeled as sets of parametric bicubic patches. There are also capabilities to transform coordinate to compute mesh/surface intersection normals, and to format input data for a transonic potential flow analysis. A graphical display of surface models and intersection normals is available. There are additional capabilities to regulate point spacing on input curves and to compute surface intersection curves. Internal details of the implementation of this system are explained, and maintenance procedures are specified

    A systematic review of worldwide cancer nursing research: 1994 to 2003

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    Kelly contributed to the conduct and choice of papers for the study, carried out a systematic review of one sixth of all the papers, contributed to the conclusion and helped to edit the final version of this paper

    Dissociation of Action and Object Naming: Evidence From Cortical Stimulation Mapping

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    This cortical stimulation mapping study investigates the neural representation of action and object naming. Data from 13 neurosurgical subjects undergoing awake cortical mapping is presented. Our findings indicate clear evidence of differential disruption of noun and verb naming in the context of this naming task. At the individual level, evidence was found for punctuate regions of perisylvian cortex subserving noun and verb function. Across subjects, however, the location of these sites varied. This finding may help explain discrepancies between lesion and functional imaging studies of noun and verb naming. In addition, an alternative coding of these data served to highlight the grammatical class vulnerability of the target response. The use of this coding scheme implicates a role for the supramarginal gyrus in verb-naming behavior. These data are discussed with respect to a functional-anatomical pathway underlying verb naming
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