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Imaging polarimetry of Comet C/2012 L2 (LINEAR)

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dc.contributor.author Roy, P. D.
dc.contributor.author Das, H. S.
dc.contributor.author Medhi, B. J.
dc.date.accessioned 2015-06-02T06:09:28Z
dc.date.available 2015-06-02T06:09:28Z
dc.date.issued 2014
dc.identifier.uri http://hdl.handle.net/123456789/1074
dc.description.abstract We present the polarimetric results and analysis of Comet C/2012 L2 (LINEAR) observed at 31°.1 phase angle before perihelion passage. The observations of the comet were carried out using ARIES Imaging Polarimeter (AIMPOL) mounted on the 1.04-m Sampurnanand telescope of ARIES, Nainital, India on 11 and 12 March, 2013 using R photometric band (ʎ = 630 nm, ∆ʎ= 120 nm). The extended coma of the comet (~65000 km) shows a significant variation in the intensity as well as polarization profile in all con- sidered directions which suggest that the dust particles originate from the active areas of the nucleus. The elongation of the coma is prominent along the Sun–comet position angle. The polarization of Comet C/ 2012 L2 (LINEAR) do not show steep radial dependence on the aperture size during both the nights of observation. A jet extended in the antisolar direction is well observed in both intensity and polarization map. en_US
dc.language.iso en_US en_US
dc.publisher Elsevier en_US
dc.relation.ispartofseries ;icarus245-241
dc.subject Comets en_US
dc.subject Dust en_US
dc.title Imaging polarimetry of Comet C/2012 L2 (LINEAR) en_US
dc.type Article en_US


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