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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4205
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dc.contributor.authorSivaram, C-
dc.date.accessioned2008-12-29T14:43:00Z-
dc.date.available2008-12-29T14:43:00Z-
dc.date.issued1987-02-
dc.identifier.citationEarth, Moon, and Planets, Vol. 37, No. 2, pp. 155 - 159en
dc.identifier.issn0167-9295-
dc.identifier.urihttp://hdl.handle.net/2248/4205-
dc.description.abstractRecent improvements in the quantitative estimates of the observed heat flow from planetary objects of the solar system may be used to put rather stringent limits on any background monopole flux. The axion flux from the giant planets is also estimated.en
dc.language.isoenen
dc.publisherD. Reidel Publishing Co.en
dc.relation.urihttp://adsabs.harvard.edu/abs/1987EM%26P...37..155Sen
dc.relation.urihttp://www.springerlink.com/content/4707188157n0h121/en
dc.subjectGas Giant Planetsen
dc.subjectHeat Fluxen
dc.subjectMagnetic Monopolesen
dc.subjectPlanetary Radiationen
dc.subjectGrand Unified Theoryen
dc.subjectNucleonsen
dc.subjectRadioactive Decayen
dc.titlePlanetary heat flow limits on monopole and axion fluxesen
dc.typeArticleen
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