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    The Magnesium Isotopologues of MgH in the A(2)Pi-X-2 Sigma(+) System 

    Hinkle, Kenneth H.; Wallace, Lloyd; Ram, Ram S.; Bernath, Peter F.; Sneden, Christopher; Lucatello, Sara (2013-08)
    Using laboratory hollow cathode spectra we have identified lines of the less common magnesium isotopologues of MgH, (MgH)-Mg-25 and (MgH)-Mg-26, in the A(2)Pi-X-2 Sigma(+) system. Based on the previous analysis of (MgH)-Mg-24, ...
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    Improved Log(gf) Values for Lines of Ti I and Abundance Determinations in the Photospheres of the Sun and Metal-Poor Star HD 84937 (Accurate Transition Probabilities for Ti I) 

    Lawler, James E.; Guzman, A.; Wood, M. P.; Sneden, Christopher; Cowan, John J. (2013-04)
    New atomic transition probability measurements for 948 lines of Ti I are reported. Branching fractions from Fourier transform spectra and from spectra recorded using a 3 m echelle spectrometer are combined with published ...
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    First Stars XVI. HST/STIS Abundances Of Heavy Elements In The Uranium-Rich Metal-Poor Star CS 31082-001 

    Mello, C. Siqueira; Spite, M.; Barbuy, B.; Spite, F.; Caffau, E.; Hill, V.; Wanajo, S.; Primas, F.; Plez, B.; Cayrel, R.; Andersen, J.; Nordstrom, B.; Sneden, Christopher; Beers, T. C.; Bonifacio, P.; Francois, P.; Molaro, P. (2013-02)
    Context. The origin and site(s) of the r-process nucleosynthesis is(are) still not known with certainty, but complete, detailed r-element abundances off er our best clues. The few extremely metal-poor (EMP) stars with large ...

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    Author
    Sneden, Christopher (3)
    Andersen, J. (1)Barbuy, B. (1)Beers, T. C. (1)Bernath, Peter F. (1)Bonifacio, P. (1)Caffau, E. (1)Cayrel, R. (1)Cowan, John J. (1)Francois, P. (1)... View MoreSubjectastronomy & astrophysics (3)
    stars: abundances (3)
    r-process-rich (2)5865 nm (1)a1d2 0.90 ev (1)absorption-spectroscopy (1)argon branching ratios (1)atomic data (1)band strengths (1)branching (1)... View MoreDate Issued
    2013 (3)
    DepartmentAstronomy (3)Has File(s)Yes (3)

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