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The kinematics of the Magellanic Clouds
Uppsala University.
1995 (English)In: ASTRONOMICAL AND ASTROPHYSICAL OBJECTIVES OF SUB-MILLIARCSECOND OPTICAL ASTROMETRY, ISSN 0074-1809, no 166, 273-282 p.Article in journal (Other scientific) Published
Abstract [en]

It is essential for our understanding of the evolution of the Magellanic System, comprising the Large and the Small Magellanic Cloud, the Intercloud or Bridge region and the Magellanic Stream, to know its motions in the past. The Clouds have a common enve

Place, publisher, year, edition, pages
KLUWER ACADEMIC PUBL , 1995. no 166, 273-282 p.
Keyword [en]
LONG-PERIOD VARIABLES; PLANETARY-NEBULAE; RADIAL-VELOCITY; CH STARS; DISTANCE; MOTION; STREAM; HALO; GAS; ABSORPTION
Identifiers
URN: urn:nbn:se:uu:diva-85375OAI: oai:DiVA.org:uu-85375DiVA: diva2:113283
Note
Addresses: Westerlund BE, UNIV UPPSALA, ASTRON OBSERV, BOX 515, S-75120 UPPSALA, SWEDEN.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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