Chemical abundances of field halo stars - Implications for the building blocks of the Milky Way
2019 ◽
Vol 14
(S351)
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pp. 24-33
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AbstractI would like to review recent efforts of detailed chemical abundance measurements for field Milky Way halo stars. Thanks to the advent of wide-field spectroscopic surveys up to a several kpc from the Sun, large samples of field halo stars with detailed chemical measurements are continuously expanding. Combination of the chemical information and full six dimensional phase-space information is now recognized as a powerful tool to identify cosmological accretion events that have built a sizable fraction of the present-day stellar halo. Future observational prospects with wide-field spectroscopic surveys and theoretical prospects with supernova nucleosynthetic yields are also discussed.
2019 ◽
Vol 14
(S353)
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pp. 71-74
Keyword(s):
2015 ◽
Vol 11
(S317)
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pp. 373-374
Keyword(s):
Keyword(s):
2016 ◽
Vol 11
(S321)
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pp. 10-12
Keyword(s):
2019 ◽
Vol 14
(S351)
◽
pp. 317-320
Keyword(s):
2019 ◽
Vol 14
(S351)
◽
pp. 155-160
2012 ◽
Vol 10
(H16)
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pp. 349-349
Keyword(s):
2020 ◽
Vol 500
(4)
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pp. 5214-5228