Azimuthal Metallicity Structure in the Milky Way Disk

15 May 2015 Balser Dana S. Wenger Trey V. Anderson L. D. Bania T. M.

Elemental abundance patterns in the Galactic disk constrain theories of the formation and evolution of the Milky Way. HII region abundances are the result of billions of years of chemical evolution... (read more)

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  • ASTROPHYSICS OF GALAXIES