Abstract
We studied stellar and interstellar data of two regions of the Large Magellanic Cloud, 30 Dor and Shapley II area. We observed the splitting of the gas into a number of separate layers. Stars are generally associated with the low-velocity component, which is behind the high-velocity component.
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© 1993 Springer-Verlag
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Martin, N., Lortet, M.C. (1993). The kinematics of red supergiants in 30 Dor and Shapley II: What for ?. In: Baschek, B., Klare, G., Lequeux, J. (eds) New Aspects of Magellanic Cloud Research. Lecture Notes in Physics, vol 416. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-56432-2_184
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DOI: https://doi.org/10.1007/3-540-56432-2_184
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