Abstract We have used Far Ultraviolet Spectroscopic Explorer (FUSE) observations of the Large Magellanic Cloud (LMC) to determine the O vi column densities in the Milky Way (MW) towards 6 LMC lines of sight. The mean column density of O vi in the MW is found to be log N(O vi)= . The results confirm the patchiness of O vi absorption in the MW and the column densities are higher or comparable to the LMC.
O vi absorption in the Milky Way along the Large Magellanic Cloud lines of sight
Advances in Space Research ; 53 , 6 ; 963-966
2013-01-01
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
O vi absorption in the Milky Way along the Large Magellanic Cloud lines of sight
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