M22: AN [Fe/H] ABUNDANCE RANGE REVEALED

Journal Article · Tue Nov 10 04:00:00 EST 2009 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/705/2/1481· OSTI ID:21378285

Da Costa, G S ^[1]; Held, E V; Gullieuszik, M ^[2]; Saviane, I ^[3]

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1. Research School of Astronomy and Astrophysics, Australian National University, Mt. Stromlo Observatory, via Cotter Rd., Weston, ACT 2611 (Australia)
2. Osservatorio Astronomico di Padova, INAF, vicolo dell'Osservatorio 5, I-35122 Padova (Italy)
3. European Southern Observatory, Casilla 19001, Santiago 19 (Chile)

Intermediate resolution spectra at the Ca II triplet have been obtained for 55 candidate red giants in the field of the globular cluster M22 with the VLT/FORS2 instrument. Spectra were also obtained for a number of red giants in standard globular clusters to provide a calibration of the observed line strengths with overall abundance [Fe/H]. For the 41 M22 member stars that lie within the V - V{sub HB} bounds of the calibration, we find an abundance distribution that is substantially broader than that expected from the observed errors alone. We argue that this broad distribution cannot be the result of differential reddening. Instead, we conclude that, as has long been suspected, M22 is similar to omega Cen in having an intrinsic dispersion in heavy element abundance. The observed M22 abundance distribution rises sharply to a peak at [Fe/H] approx-1.9 with a broad tail to higher abundances: the highest abundance star in our sample has [Fe/H] approx-1.45 dex. If the unusual properties of omega Cen have their origin in a scenario in which the cluster is the remnant nucleus of a disrupted dwarf galaxy, then such a scenario likely also applies to M22.

• OSTI ID: 21378285
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 2 Vol. 705; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
ABUNDANCE
CALIBRATION
ELEMENT ABUNDANCE
GALAXIES
SPECTRA
STARS