Abundance patterns in the low-metallicity emission-line galaxies from the Early Data Release of the Sloan Digital Sky Survey

Details Abundance patterns in the low-metallicity emission-line galaxies from the Early Data Release of the Sloan Digital Sky Survey Abundance patterns in the low-metallicity emission-line galaxies from the Early Data Release of the Sloan Digital Sky Survey

2003-11-25

arxiv.org/abs/astro-ph/0311564v1

Astron.Astrophys. 415 (2004) 87-94

Astronomy and Astrophysics

Astrophysics

8 pages, 7 figures, accepted for publication in A&A

Scientific paper

10.1051/0004-6361:20034101

We have derived element abundances in 310 emission-line galaxies from the Early Data Release of the Sloan Digital Sky Survey (SDSS) for which the [O {\sc iii}] 4363 emission line was detected, allowing abundance determination by direct methods. We found no extremely metal-deficient galaxy (Z

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