dc.contributor.author |
Murthy, M |
|
dc.date.accessioned |
2008-07-17T07:05:11Z |
|
dc.date.available |
2008-07-17T07:05:11Z |
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dc.date.issued |
2002-06 |
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dc.identifier.citation |
Journal of Astrophysics and Astronomy, Vol. 23, No. 1-2, pp. 23 – 26 |
en |
dc.identifier.issn |
0250-6335 |
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dc.identifier.uri |
http://hdl.handle.net/2248/2721 |
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dc.description.abstract |
We have examined 426 Voyager fields distributed across the sky for O VI (1032/1038 Å) emission from the Galactic diffuse interstellar medium. No such emission was detected in any of our observed fields. Our most constraining limit was a 90% confidence upper limit of 2600 photons cm-2 sr-1 s-1 on the doublet emission in the direction (l, b) = (117.3, 50.6). Combining this with an absorption line measurement in nearly the same direction allows us to place an upper limit of 0.01 cm-3 on the electron density of the hot gas in this direction. We have placed 90% confidence upper limits of less than or equal to 10,000 photons cm-2 sr-1 s-1 on the O VI emission in 16 of our 426 observations. |
en |
dc.format.extent |
29648 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Indian Academy of Sciences |
en |
dc.relation.uri |
http://www.ias.ac.in/jaa/marjun2002/absmarjun.htm#Jaa295 |
en |
dc.subject |
Galaxy: Halo ISM: general |
en |
dc.title |
Upper Limits on O VI Emission from Voyager Observations |
en |
dc.type |
Article |
en |