Chemical Abundances of DEEP2 Star-forming Galaxies at 1.0<z<1.5

Details Chemical Abundances of DEEP2 Star-forming Galaxies at 1.0<z<1.5 Chemical Abundances of DEEP2 Star-forming Galaxies at 1.0<z<1.5

2005-09-05

arxiv.org/abs/astro-ph/0509102v1

Astrophys.J.635:1006-1021,2005

Astronomy and Astrophysics

Astrophysics

19 pages including 5 figures. Accepted for publication in ApJ

Scientific paper

10.1086/497630

We present the results of near-infrared spectroscopic observations for a sample of 12 star-forming galaxies at 1.01 DEEP2 galaxies in our sample are significantly offset from the excitation sequence observed in nearby HII regions and SDSS emission-line galaxies. This offset implies that physical conditions are different in the HII regions of distant galaxies hosting intense star formation, and may affect the chemical abundances derived from strong-line ratios for such objects (Abridged).

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