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Lifting the Veil on Ultra Metal-Poor Stars in the Outermost Halo

Published online by Cambridge University Press:  02 August 2018

Jinmi Yoon
Affiliation:
Department of Physics, University of Notre Dame, Notre Dame, IN, USA email: [email protected] JINA Center for the Evolution of the Elements, Notre Dame, IN, USA
Devin D. Whitten
Affiliation:
Department of Physics, University of Notre Dame, Notre Dame, IN, USA email: [email protected] JINA Center for the Evolution of the Elements, Notre Dame, IN, USA
Timothy C. Beers
Affiliation:
Department of Physics, University of Notre Dame, Notre Dame, IN, USA email: [email protected] JINA Center for the Evolution of the Elements, Notre Dame, IN, USA
Vinicius M. Placco
Affiliation:
Department of Physics, University of Notre Dame, Notre Dame, IN, USA email: [email protected] JINA Center for the Evolution of the Elements, Notre Dame, IN, USA
Young Sun Lee
Affiliation:
Department of Astronomy & Space Science, Chungnam National Univ., Daejeon, South Korea
Sarah Dietz
Affiliation:
Department of Physics, University of Notre Dame, Notre Dame, IN, USA email: [email protected] JINA Center for the Evolution of the Elements, Notre Dame, IN, USA
Dmitrii Gudin
Affiliation:
Department of Physics, University of Notre Dame, Notre Dame, IN, USA email: [email protected] JINA Center for the Evolution of the Elements, Notre Dame, IN, USA
Kaitlin C. Rasmussen
Affiliation:
Department of Physics, University of Notre Dame, Notre Dame, IN, USA email: [email protected] JINA Center for the Evolution of the Elements, Notre Dame, IN, USA
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Abstract

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The study of extremely metal-poor (EMP; [Fe/H] <−3.0) and ultra metal-poor (UMP; [Fe/H] <−4.0) stars is crucial for better understanding first-star nucleosynthesis and constraining the initial mass function in the early Universe. However, UMP stars discovered in the past 25 years only number ~25. A few recent theoretical studies have pointed out that there is likely to exist large numbers of EMP and UMP stars in the periphery of the Galactic halo, at distances exceeding 30-50 kpc. We present identifications of several new EMP/UMP stars and introduce a survey to expedite discovering hundreds to thousands of EMP/UMP stars in the outermost halo (as well as in the local volume) over the next few years, which could revolutionize chemical-evolution studies of the Galaxy.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Beers, T. C. & Christlieb, N., 2005, ARAA, 43, 531Google Scholar
Beers, T. C., Norris, J. E., Placco, V. M., et al. 2014, ApJ, 794, 58Google Scholar
Lee, Y. S., Beers, T. C., Sivarani, T., et al. 2008, ApJ, 136, 2022Google Scholar
Placco, V. M., Frebel, A., Beers, T. C. & Stancliffe, R. J., 2014, ApJ, 797, 21Google Scholar
Plez, B. & Cohen, J. G., 2005, AA, 434, 1117Google Scholar
Yoon, J., Beers, T. C., Placco, V. M. et al. 2016, AJ, 833, 20Google Scholar