Abstract
Linear polarization observations were carried out on comet C/2000 WM1 with the 1.2 m telescope at Mt. Abu Observatory during November 2001 and March 2002. The observations in November were at low phase angle (<22°) when the polarization is negative and where the data for most of the comets are rather meager. The observations during March were made when the phase angle was ∼47°. Observations were conducted through the 1HW narrow band and BVR broad band filters. Based on these polarization observations we infer that the comet C/2000 WM1 belongs to high polarization class i.e. the dusty comet family.
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CITATION STYLE
Joshi, U. C., Baliyan, K. S., & Ganesh, S. (2003). Polarization studies of comet C/2000 WM1 (LINEAR). Astronomy and Astrophysics, 405(3), 1129–1135. https://doi.org/10.1051/0004-6361:20030684
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