The metallicity extremes of the Sagittarius dSph: SALT spectroscopy of PNe

Type Journal Article
Names Alexei Y. Kniazev, Albert A. Zijlstra, Eva K. Grebel, Leonid S. Pilyugin, Simon Pustilnik, Petri Väisänen, David Buckley, Yas Hashimoto, Nicola Loaring, Encarni Romero, Martin Still, Eric B. Burgh, Kenneth Nordsieck
Publication Monthly Notices of the Royal Astronomical Society
Volume 388
Issue 4
Pages 1667-1678
Date August 1, 2008
Short Title The metallicity extremes of the Sagittarius dSph
URL http://adsabs.harvard.edu/abs/2008MNRAS.388.1667K
Library Catalog NASA ADS
Abstract In this work we present the first spectroscopic results obtained with the Southern African Large Telescope (SALT) during its performance-verification phase. We find that the Sagittarius dwarf spheroidal galaxy (Sgr) contains a youngest stellar population with [O/H] ~ -0.2 and age t > 1Gyr, and an oldest population with [O/H]= -2.0. The values are based on spectra of two planetary nebulae (PNe), using empirical abundance determinations. We calculated abundances for O, N, Ne, Ar, S, Cl, Fe, C and He. We confirm the high abundances of PN StWr2-21 with 12 + log(O/H) = 8.57 +/- 0.02 dex. The other PN studied, BoBn1, is an extraordinary object in that the neon abundance exceeds that of oxygen. The abundances of S, Ar and Cl in BoBn1 yield the original stellar metallicity, corresponding to 12 + log(O/H) = 6.72 +/- 0.16 dex which is 1/110 of the solar value. The actual [O/H] is much higher: third dredge-up enriched the material by a factor of ~12 in oxygen, ~240 in nitrogen and ~70 in neon. Neon as well as nitrogen and oxygen content may have been produced in the intershell of low-mass asymptotic giant branch (AGB) stars. Well defined broad WR lines are present in the spectrum of StWr2-21 and absent in the spectrum of BoBn1. This puts the fraction of [WR]-type central PNe stars to 67 per cent for dSph galaxies. Based on observations obtained with Southern African Large Telescope (SALT). E-mail: akniazev@saao.ac.za (AYK); a.zijlstra@manchester.ac.uk (AAZ)
Tags Stars: Abundances, galaxies: individual: Sagittarius dwarf spheroidal, planetary nebulae: general, stars: mass-loss
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