Near-Infrared Spectroscopy of 0.4<z<1.0 CFRS Galaxies: Oxygen Abundances, SFRs and Dust

Using new J-band VLT-ISAAC and Keck-NIRSPEC spectroscopy, we have measured Halpha and [NII] line fluxes for 0.47 0.1 for most (but not all) of the CFRS galaxies indicate that they lie on the high-metallicity branch of the R23 calibration; d) about one third of the 0.47

Keywords:

• chemical evolution
• Galaxy
• Spectroscopy
• Near-infrared spectroscopy
• Dwarf galaxy
• Oxygen
• Astrophysics
• Star formation
• Metallicity
• Physics

• Correction
• Source
• Cite
• Save
• Machine Reading By IdeaReader