期刊
ASTROPHYSICAL JOURNAL LETTERS
卷 726, 期 2, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/2041-8205/726/2/L20
关键词
Galaxy: abundances; Galaxy: bulge; infrared: stars; stars: abundances; stars: late-type; techniques: spectroscopic
资金
- Istituto Nazionale di Astrofisica (INAF)
- Ministero dell'Istruzione, Universita a e Ricerca (MIUR)
- Agenzia Spaziale Italiana (ASI) [ASI/INAF I/009/10/0]
- National Science Foundation [AST 07-09479]
We present the chemical abundance analysis of 33 red giant stars belonging to the complex stellar system Terzan 5. We confirm the discovery of two stellar populations with distinct iron abundances: a relatively metal-poor component with [Fe/H] = -0.25 +/- 0.07 rms and another component with [Fe/H] = +0.27 +/- 0.04 rms, exceeding in metallicity any known Galactic globular cluster (GC). The two populations also show different [alpha/Fe] abundance ratios. The metal-poor component has an average [alpha/Fe] = +0.34 +/- 0.06 rms, consistent with the canonical scenario for rapid enrichment by core collapse supernovae (SNe). The metal-rich component has [alpha/Fe] = +0.03 +/- 0.04 rms, suggesting that the gas from which it formed was polluted by both type II and type Ia SNe on a longer timescale. Neither of the two populations shows evidence of the [Al/Fe] over [O/Fe] anti-correlation that is typically observed in Galactic GCs. Because these chemical abundance patterns are unique, we propose that Terzan 5 is not a true GC, but a stellar system with a much more complex history of star formation and chemical enrichment.
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