9,315 research outputs found

    Why Are Ring Galaxies Interesting?

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    Compared with ordinary spirals, the ISM in ring galaxies experiences markedly different physical conditions and evolution. As a result, ring galaxies provide interesting perspectives on the triggering/quenching of large scale star formation and the destructive effects of massive stars on molecular cloud complexes. We use high resolution radio, sub-millimeter, infrared, and optical data to investigate the role of gravitational stability in star formation regulation, factors influencing the ISM's molecular fraction, and evidence of peculiar star formation laws and efficiencies in two highly evolved ring galaxies: Cartwheel and the Lindsay-Shapley ring.Comment: 6 pages with 4 figures (2 color). To appear in the conference proceedings for "Galaxy Wars: Stellar Populations and Star Formation in Interacting Galaxies"

    Feminist Geopolitics: Material States

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    Determinants and outcomes of motivation in health professions education: a systematic review based on self-determination theory

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    Purpose: This study aimed at conducting a systematic review in health professions education of determinants, mediators and outcomes of students’ motivation to engage in academic activities based on the self-determination theory’s perspective. Methods: A search was conducted across databases (MEDLINE, CINHAL, EMBASE, PsycINFO, and ERIC databases), hand-search of relevant journals, grey literature, and published research profile of key authors. Quantitative and qualitative studies were included if they reported research in health professions education focused on determinants, mediators, and/or outcomes of motivation from the self-determination and if meeting the quality criteria. Results: A total of 17 studies met the inclusion and quality criteria. Articles retrieved came from diverse locations and mainly from medical education and to a lesser extent from psychology and dental education. Intrapersonal (gender and personality traits) and interpersonal determinants (academic conditions and lifestyle, qualitative method of selection, feedback, and an autonomy supportive learning climate) have been reported to have a positive influence on students’ motivation to engage in academic activities. No studies were found that tested mediation effects between determinants and students’ motivation. In turn, students’ self-determined motivation has been found to be positively associated with different cognitive, affective, and behavioural outcomes. Conclusion: This study has found that generally, motivation could be enhanced by changes in the educational environment and by an early detection of students’ characteristics. Doing so may support future health practitioners’ self-determined motivation and positively influence how they process information and their emotions and how they approach their learning activities

    Molecular Gas and Star Formation in the Cartwheel

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    Atacama Large Millimeter/submillimeter Array (ALMA) 12CO(J=1-0) observations are used to study the cold molecular ISM of the Cartwheel ring galaxy and its relation to HI and massive star formation (SF). CO moment maps find (2.69±0.05)×109(2.69\pm0.05)\times10^{9} M⊙_{\odot} of H2_2 associated with the inner ring (72%) and nucleus (28%) for a Galactic I(CO)-to-N(H2) conversion factor (αCO\alpha_{\rm CO}). The spokes and disk are not detected. Analysis of the inner ring's CO kinematics show it to be expanding (Vexp=68.9±4.9V_{\rm exp}=68.9\pm4.9 km s−1^{-1}) implying an ≈70\approx70 Myr age. Stack averaging reveals CO emission in the starburst outer ring for the first time, but only where HI surface density (ΣHI\Sigma_{\rm HI}) is high, representing MH2=(7.5±0.8)×108M_{\rm H_2}=(7.5\pm0.8)\times10^{8} M⊙_{\odot} for a metallicity appropriate αCO\alpha_{\rm CO}, giving small ΣH2\Sigma_{\rm H_2} (3.73.7 M⊙_{\odot} pc−2^{-2}), molecular fraction (fmol=0.10f_{\rm mol}=0.10), and H2_2 depletion timescales (τmol≈50−600\tau_{\rm mol} \approx50-600 Myr). Elsewhere in the outer ring ΣH2≲2\Sigma_{\rm H_2}\lesssim 2 M⊙_{\odot} pc−2^{-2}, fmol≲0.1f_{\rm mol}\lesssim 0.1 and τmol≲140−540\tau_{\rm mol}\lesssim 140-540 Myr (all 3σ3\sigma). The inner ring and nucleus are H2_2-dominated and are consistent with local spiral SF laws. ΣSFR\Sigma_{\rm SFR} in the outer ring appears independent of ΣH2\Sigma_{\rm H_2}, ΣHI\Sigma_{\rm HI} or ΣHI+H2\Sigma_{\rm HI+H_2}. The ISM's long confinement in the robustly star forming rings of the Cartwheel and AM0644-741 may result in either a large diffuse H2_2 component or an abundance of CO-faint low column density molecular clouds. The H2_2 content of evolved starburst rings may therefore be substantially larger. Due to its lower ΣSFR\Sigma_{\rm SFR} and age the Cartwheel's inner ring has yet to reach this state. Alternately, the outer ring may trigger efficient SF in an HI-dominated ISM.Comment: 10-pages text; 5-figure

    Spitzer Observations of Tidal Dwarf Galaxies

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    We present Spitzer observations of Tidal Dwarf Galaxies (TDGs) in three interacting systems: NGC 5291, Arp 105 & Stephan’s Quintet. The spectra show bright emission from polyaromatic hydrocarbons (PAHs), nebular lines and warm molecular hydrogen, characteristic of recent episodes of star formation. The PAH emission that falls in the IRAC 8.0 µm band leads to the TDGs having an extremely red IRAC color, with [4.5] − [8.0] \u3e 3. The emission from PAHs is characterized by a model with mainly neutral 100-C PAH atoms
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