The Physical Conditions of a Lensed Star-forming Galaxy at z = 1.7

We report rest-frame optical Keck/NIRSPEC spectroscopy of the bright lensed galaxy RCSGA 032727-132609 at z = 1.7037. From precise measurements of the nebular lines, we infer a number of physical properties: redshift, extinction, star formation rate, ionization parameter, electron density, electron...

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Veröffentlicht in:The Astrophysical journal 2011-05, Vol.732 (1), p.59-jQuery1323909208223='48'
Hauptverfasser: Rigby, J. R, Wuyts, E, Gladders, M. D, Sharon, K, Becker, G. D
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Sprache:eng
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Zusammenfassung:We report rest-frame optical Keck/NIRSPEC spectroscopy of the bright lensed galaxy RCSGA 032727-132609 at z = 1.7037. From precise measurements of the nebular lines, we infer a number of physical properties: redshift, extinction, star formation rate, ionization parameter, electron density, electron temperature, oxygen abundance, and N/O, Ne/O, and Ar/O abundance ratios. The limit on [O III] 4363 A tightly constrains the oxygen abundance via the 'direct' or Te method, for the first time in an average-metallicity galaxy at z ~ 2. We compare this result to several standard 'bright-line' O abundance diagnostics, thereby testing these empirically-calibrated diagnostics in situ. Finally, we explore the positions of lensed and unlensed galaxies in standard diagnostic diagrams, and the diversity of ionization conditions and mass-metallicity ratios at z = 2.
ISSN:0004-637X
1538-4357
DOI:10.1088/0004-637X/732/1/59