2011ApJ...732...59R


Query : 2011ApJ...732...59R

2011ApJ...732...59R - Astrophys. J., 732, 59 (2011/May-1)

The physical conditions of a lensed star-forming galaxy at z = 1.7.

RIGBY J.R., WUYTS E., GLADDERS M.D., SHARON K. and BECKER G.D.

Abstract (from CDS):

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 Å tightly constrains the oxygen abundance via the "direct" or Temethod, 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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Journal keyword(s): galaxies: abundances - galaxies: evolution - galaxies: high-redshift - gravitational lensing: strong

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME 8 O'Clock Arc blu 00 22 40.77984 +14 31 13.9548           ~ 66 0
2 RCSGA J032727-132609 G 03 27 27.3 -13 26 09         21.39 ~ 31 1
3 HD 23683 * 03 46 31.6776769416 -15 14 55.988326860   8.23 8.19     A0V 13 0
4 M 42 HII 05 35 16.8 -05 23 15           ~ 4411 0
5 [DAA2009] SDSS J090002.79+223403.6 source G 09 00 02.79 +22 34 03.6           ~ 14 1
6 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6
7 CSWA 1 gLS 11 48 33.10 +19 30 03.2           ~ 90 0
8 NAME the Clone gLS 12 06 02.09 +51 42 29.5           ~ 45 0
9 ACO 1689 ClG 13 11 29.5 -01 20 28           ~ 1178 0
10 NAME MS 1512-cB58 AGN 15 14 22.2751 +36 36 25.674     20.64   20.35 ~ 326 0

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