Fig. 1 from The Luminosity‐Metallicity Relation, Effective Yields, and Metal Loss in Spiral and Irregular Galaxies

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

The Luminosity‐Metallicity Relation, Effective Yields, and Metal Loss in Spiral and Irregular Galaxies

Authors: Donald R. Garnett

Garnett 2002 The Astrophysical Journal 581 1019.

Provider: AAS Journals

Caption: Fig. 1.

(a) Correlation between O/H at the disk half‐light radius R_eff and absolute B magnitude for spiral and irregular galaxies. (b) O/H at R_eff vs. rotation speed V_rot for the same sample. For spirals the rotation speed is taken to be that on the flat part of the rotation curve.

Other Images in This Article

Copyright and Terms & Conditions