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.
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CITATION STYLE
APA
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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