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arXiv · 1307.6928

O~{\small VI} absorption in the Milky Way along the Large Magellanic Cloud lines of sight

Rathin Sarma·Amit Pathak·Ananta C. Pradhan·Jayant Murthy·Jayanta K. Sarma
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Abstract

We have used \textit{Far Ultraviolet Spectroscopic Explorer (FUSE)} observations of the Large Magellanic Cloud (LMC) to determine the O {\small VI} column densities in the Milky Way (MW) towards 6 LMC lines of sight. The mean column density of O {\small VI} in the MW is found to be log N(O {\small VI})=14.257$_{-0.084}^{+0.096}$. The results confirm the patchiness of O {\small VI} absorption in the MW and the column densities are higher or comparable to the LMC.

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Rathin Sarma, Amit Pathak, Ananta C. Pradhan, Jayant Murthy, Jayanta K. Sarma. 2013-07-26. O~{\small VI} absorption in the Milky Way along the Large Magellanic Cloud lines of sight. https://doi.org/10.1016/j.asr.2013.06.020

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