281 research outputs found

    A New Color-Magnitude Diagram for Palomar 11

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    We present new photometry for the Galactic thick disk globular cluster Palomar 11 extending well past the main sequence turn-off in the V and I bands. This photometry shows noticeable red giant and subgiant branches. The difference in magnitude between the red horizontal branch (red clump) and the subgiant branch is used to determine that Palomar 11 has an age of 10.4+/-0.5 Gyr. The red clump is used to derive a distance d_\sun=14.3+/-0.4 kpc, and a mean cluster reddening of E(V-I)=0.40+/-0.03. There is differential reddening across the cluster, of order \delta E(V-I)~0.07. The colour magnitude diagram of Palomar 11 is virtually identically to that of the thick disk globular cluster NGC 5927, implying that these two clusters have a similar age and metallicity. Palomar 11 has a slightly redder red giant branch than 47 Tuc, implying that Palomar 11 is 0.15 dex more metal-rich, or 1 Gyr older than 47 Tuc. Ca II triplet observations (Rutledge et al. 1997) favour the hypothesis that Palomar 11 is the same age as 47 Tuc, but slightly more metal-rich.Comment: to appear in AJ (19 pages, 4 B&W figures, 1 colour figure

    The influence of personal characteristics on perioperative nurses' perceived competence: Implications for workforce planning

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    Objective: To examine the influence of personal characteristics on perioperative nurses' perceived competence. Design: A cross-sectional survey design was used. Setting: A census of 3,209 operating room nurses who were members of the Australian College of Operating Room Nurses across all Australian states and territories was invited to participate. Primary Outcome Measure: The Perceived Perioperative Competence Scale-Revised, a 40-item survey consisting of six subscales measuring the dimensions of perioperative competence was used. Results: A total of 1,044 usable surveys were analysed representing 32.5% of the accessible population. Across the six subscales, demographic predictors accounted for 5% to 33% of the variance in nurses' perceived perioperative competence. Conclusions: These results may inform workforce planning initiatives designed to address the needs of this diverse specialty group. Efforts to retain older nurses need to be centered on redesigning workplaces, increased remuneration and professional recognition, and integrating technology to promote efficiency and safety. Workforce planning should include strategies such as creating academic partnerships with universities, to provide perioperative nurses access to specialty education and advanced skills programs

    Direct measurement of the 14N(p,g)15O S-factor

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    We have measured the 14N(p,g)15O excitation function for energies in the range E_p = 155--524 keV. Fits of these data using R-matrix theory yield a value for the S-factor at zero energy of 1.64(17) keV b, which is significantly smaller than the result of a previous direct measurement. The corresponding reduction in the stellar reaction rate for 14N(p,g)15O has a number of interesting consequences, including an impact on estimates for the age of the Galaxy derived from globular clusters.Comment: 5 pages, 3 figures, submitted to Phys. Rev. Let

    Stellar Population Models and Individual Element Abundances. I. Sensitivity of Stellar Evolution Models

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    Integrated light from distant galaxies is often compared to stellar population models via the equivalent widths of spectral features—spectral indices—whose strengths rely on the abundances of one or more elements. Such comparisons hinge not only on the overall metal abundance, but also on relative abundances. Studies have examined the influence of individual elements on synthetic spectra but little has been done to address similar issues in the stellar evolution models that underlie most stellar population models. Stellar evolution models will primarily be influenced by changes in opacities. In order to explore this issue in detail, 12 sets of stellar evolution tracks and isochrones have been created at constant heavy element mass fraction Z that self-consistently account for varying heavy element mixtures. These sets include scaled-solar, α-enhanced, and individual cases where the elements C, N, O, Ne, Mg, Si, S, Ca, Ti, and Fe have been enhanced above their scaled-solar values. The variations that arise between scaled-solar and the other cases are examined with respect to the H-R diagram and main-sequence lifetimes
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