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.
CITATION STYLE
Welty, D. E., Frisch, P. C., Hobbs, L. M., York, D. G., Blades, J. C., Lauroesch, J. T., & Sonneborn, G. (1999). Interstellar Abundances in the Magellanic Clouds. Symposium - International Astronomical Union, 190, 277–278. https://doi.org/10.1017/s0074180900118030
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