Proceedings of the Workshop
"The Magellanic Clouds and Other Dwarf Galaxies"
of the Bonn/Bochum-Graduiertenkolleg

The Kinematic Structure of the Supergiant Shell LMC 2

Sean D. Points


Fig. 1
Fig. 1. Image of the three echelle cuts toward LMC 2. The zero-point in the spatial direction for each echellogram is
(a) α2000 = 5h 42m 10s; δ2000 = -69° 13' 28",
(b) α2000 = 5h 45m 33s; δ2000 = -69° 25' 05", and
(c) α2000 = 5h 43m 04s; δ2000 = -69° 36' 05".
The velocity zero-points is taken to be the geocoronal Halpha line

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First version: 07thJuly,1998
Last update: 30thSeptember,1998

Jochen M. Braun   &   Tom Richtler
 (E-Mail: jbraun|richtler@astro.uni-bonn.de)