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 |