Issue |
A&A
Volume 405, Number 3, July III 2003
|
|
---|---|---|
Page(s) | 1129 - 1135 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361:20030684 | |
Published online | 30 June 2003 |
Polarization studies of comet C/2000 WM1 (LINEAR)
Physical Research Laboratory, Ahmedabad 380009, India
Corresponding author: U. C. Joshi, joshi@prl.ernet.in
Received:
25
June
2002
Accepted:
23
April
2003
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 (<) 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 IHW 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.
Key words: comets: individual: C/2000 WM1 (LINEAR)
© ESO, 2003
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