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Interstellar Abundances in the Magellanic Clouds
Published online by Cambridge University Press: 25 May 2016
Abstract
We discuss the relative gas-phase abundances found for the predominantly neutral interstellar clouds — located in the Galactic disk and halo, in the LMC or SMC, and (perhaps) in between — along the lines of sight to Sk 108 in the SMC and to SN 1987A in the LMC.
- Type
- Part 4. Detailed Chemical Abundances
- Information
- Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 277 - 278
- Copyright
- Copyright © Astronomical Society of the Pacific 1999