O VI absorption in the milky way along the large magellanic cloud lines of sight

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6550

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DC Field	Value	Language
dc.contributor.author	Sarma, R	-
dc.contributor.author	Pathak, A	-
dc.contributor.author	Pradhan, A. C	-
dc.contributor.author	Murthy, J	-
dc.contributor.author	Sarma, J. K	-
dc.date.accessioned	2014-02-28T11:23:53Z	-
dc.date.available	2014-02-28T11:23:53Z	-
dc.date.issued	2014-03-15	-
dc.identifier.citation	Advances in Space Research, Vol. 53, No. 6, pp. 963–966	en
dc.identifier.issn	0273-1177	-
dc.identifier.uri	http://hdl.handle.net/2248/6550	-
dc.description	Restricted Access	en
dc.description.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) = View the MathML source14.257-0.084+0.096. The results confirm the patchiness of O vi absorption in the MW and the column densities are higher or comparable to the LMC.	en
dc.language.iso	en	en
dc.publisher	Elsevier B.V	en
dc.relation.uri	http://dx.doi.org/10.1016/j.asr.2013.06.020	en
dc.rights	© Elsevier B.V.	en
dc.subject	ISM:atoms	en
dc.subject	ISM:galaxies	en
dc.subject	Milky Way	en
dc.title	O VI absorption in the milky way along the large magellanic cloud lines of sight	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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