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' |
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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. |
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ISSN: | 0004-637X 1538-4357 |
DOI: | 10.1088/0004-637X/732/1/59 |