Properties and Origin of the High-Velocity Gas Toward the Large Magellanic Cloud

Details Properties and Origin of the High-Velocity Gas Toward the Large Magellanic Cloud Properties and Origin of the High-Velocity Gas Toward the Large Magellanic Cloud

2009-07-14

arxiv.org/abs/0907.2416v1

Astrophys.J.702:940-954,2009

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

Accepted for publication in the ApJ

Scientific paper

10.1088/0004-637X/702/2/940

In the spectra of 139 early-type Large Magellanic Cloud (LMC) stars observed with FUSE and with deep radio Parkes HI 21-cm observations along those stars, we search for and analyze the absorption and emission from high-velocity gas at +9010^6 M_sun) HVC complex that is linked to stellar feedback occurring in a dwarf spiral galaxy.

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