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The RAVE survey: Rich in very metal-poor stars

Abstract:

Very metal-poor stars are of obvious importance for many problems in chemical evolution, star formation, and galaxy evolution. Finding complete samples of such stars which are also bright enough to allow high-precision individual analyses is of considerable interest. We demonstrate here that stars with iron abundances [Fe/H] < -2 dex, and down to below -4 dex, can be efficiently identified within the Radial Velocity Experiment (RAVE) survey of bright stars, without requiring additional con...

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Publisher copy:
10.1088/2041-8205/724/1/L104

Authors


Journal:
Astrophysical Journal Letters More from this journal
Volume:
724
Issue:
1 PART 2
Publication date:
2010-11-20
DOI:
EISSN:
2041-8213
ISSN:
2041-8205
Language:
English
Keywords:
Pubs id:
pubs:212413
UUID:
uuid:6693db23-1b13-4ef6-b21e-48fa71d6ddd1
Local pid:
pubs:212413
Source identifiers:
212413
Deposit date:
2012-12-19

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