Is there a gaseous halo around the Large Magellanic Cloud ?
DOI: 10.1086/160014
Bibcode: 1982ApJ...257..587F
Feitzinger, J. V.; Schmidt-Kaler, T.
Germany
Abstract
Arguments are given which show that the evidence for a hot gaseous halo around the Large Magellanic Cloud is not at all conclusive. The observations of interstellar lines in the UV, optical, and radio domain are well represented by a kinematic model of the LMC with a warped, two-layer structure.
1982
•
The Astrophysical Journal
IUE
16