Is there a gaseous halo around the Large Magellanic Cloud

Details Is there a gaseous halo around the Large Magellanic Cloud Is there a gaseous halo around the Large Magellanic Cloud

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...257..587f&link_type=abstract

Astrophysical Journal, Part 1, vol. 257, June 15, 1982, p. 587-591

Astronomy and Astrophysics

Astrophysics

13

Galactic Structure, Halos, Interstellar Gas, Magellanic Clouds, Ultraviolet Spectra, Galactic Rotation, Hydrogen Clouds, Radial Velocity, Spectral Line Width, Ultraviolet Absorption

Scientific paper

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.

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