Investigations of the Rotation Pole from the Morphology of Dust Fans of Comet 81P/Wild 2

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3585

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DC Field	Value	Language
dc.contributor.author	Vasundhara, R	-
dc.contributor.author	Chakraborty, P	-
dc.date.accessioned	2008-09-12T11:19:20Z	-
dc.date.available	2008-09-12T11:19:20Z	-
dc.date.issued	2004-12	-
dc.identifier.citation	Astrophysical Journal, Vol. 616, No. 2, Part 1, pp. 1278 - 1283	en
dc.identifier.issn	0004-637X	-
dc.identifier.uri	http://hdl.handle.net/2248/3585	-
dc.description.abstract	Investigations of the dust morphology of comet 81P/Wild 2 in the I- and R-band images obtained on 1997 May 15 from the Vainu Bappu Observatory, Kavalur, India, are presented. We model the trajectories of dust grains ejected from distributed sources on this comet to explain the morphology of the fans in these images and in the published images by Schulz and coworkers. We derive the pole position of αp=297deg+/-5deg and δp=-10deg+/-5deg. Broad sources at +80deg+/-5deg and -25deg+/-5deg latitudes best explain the northern and southern fans, respectively.	en
dc.language.iso	en	en
dc.publisher	The American Astronomical Society	en
dc.relation.uri	http://www.journals.uchicago.edu/doi/abs/10.1086/424953	en
dc.subject	Comets: General	en
dc.subject	Comets: Individual: Name: 81P/Wild 2	en
dc.subject	Space Vehicles	en
dc.title	Investigations of the Rotation Pole from the Morphology of Dust Fans of Comet 81P/Wild 2	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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