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Hi-distribution, kinematics and geometry of the Large Magellanic Cloud
Published online by Cambridge University Press: 19 July 2016
Abstract
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Here we discuss current observational data on, and the distribution of, neutral hydrogen in the Large Magellanic Cloud (LMC).
- Type
- Large-Scale Structure and Kinematics
- Information
- Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 63 - 67
- Copyright
- Copyright © Kluwer 1991
References
Cohen, R.S., Dame, T.M., Garay, G., Montani, J., Rubio, M., Thaddeus, P. (1988),
Astrophys. J.
331, L95.CrossRefGoogle Scholar
Feitzinger, J.V., Isserstedt, J., Schmidt-Kaler, Th. (1977),
Astron. Astrophys.
57, 265.Google Scholar
Martin, N., Prévot, L., Rousseau, J. (1989),
Proc. Europ. Colloq. Recent Developments of Magellanic Cloud Research
, de Boer, K.S. et al. (eds.) (Observatoire de Paris: Paris), p.155.Google Scholar
Meaburn, J., Marston, A.P., McGee, R.X., Newton, L.M. (1987),
Mon. Not. R. Astron. Soc.
225, 591.Google Scholar
Rohlfs, K., Kreitschmann, J., Siegman, B.C., Feitzinger, J.V. (1984),
Astron. Astrophys.
137, 343.Google Scholar
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