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Molecular emission from the head of comet P/Crommelin 1818 I

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dc.contributor.author Goraya, P. S.
dc.contributor.author Rautela, B. S.
dc.contributor.author Sanwal, B. B.
dc.date.accessioned 2010-07-27T08:17:07Z
dc.date.available 2010-07-27T08:17:07Z
dc.date.issued 1984
dc.identifier.citation This article downloded from ADS Free Online Journal en_US
dc.identifier.uri http://hdl.handle.net/123456789/713
dc.description.abstract The comet P/Crommelin has attracted the attention of a larga of scientists during its recent apparition in 1984 February. During its earlier returns (in 1818, 1873, 1928, and 1956) the motion of Comet Crommelin holds the of Comet Crommelin is to exercise the entire International Halley Watch (IHW) prior to the observations of Comet Halley. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries jba94-186
dc.subject Comet P/Crommelin 1818 I en_US
dc.title Molecular emission from the head of comet P/Crommelin 1818 I en_US
dc.type Article en_US


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