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Article
PRODUCTION OF MILKY-WAY STRUCTURE BY THE MAGELLANIC-CLOUDS
ASTROPHYSICAL JOURNAL
  • MD Weinberg
Publication Date
1995
Abstract
Previous attempts at disturbing the galactic disk by the Magellanic Clouds relied on direct tidal forcing. However, by allowing the halo to actively respond rather than remain a rigid contributor to the rotation curve, the Clouds may produce a wake in the halo which then distorts the disk. Recent work reported here suggests that the Magellanic Clouds use this mechanism to produce disk distortions sufficient to allow for both the radial location, position angle and sign of the HI warp and observed anomalies in stellar kinematics toward the galactic anticenter and LSR motion.
Comments
This is a pre-published version which is collected from arXiv link.
Pages
L31-L34
Citation Information
MD Weinberg. "PRODUCTION OF MILKY-WAY STRUCTURE BY THE MAGELLANIC-CLOUDS" ASTROPHYSICAL JOURNAL Vol. 455 Iss. 1 (1995)
Available at: http://works.bepress.com/martin_weinberg/40/