Optical polarimetry and photometry of comet 17P/Holmes

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

11pages, 7 figures, accepted for publication in MNRAS

Scientific paper

Comet 17P/Holmes was observed for linear polarisation using the optical polarimeter mounted on the 1.2m telescope atop Gurushikhar peak near Mt. Abu during the period November-December 2007. Observations were conducted through the IHW narrow band (continuum) filters. During the observing run the phase angle was near $13^{\circ}$ at which the comet showed negative polarisation. On the basis of the observed polarisation data we find comet 17P/Holmes to be a typical comet with usual dust characteristics. We note that radial rate of change of brightness in coma in red band is higher than that in blue band; it has decreased by a factor of 3.6 and 2.5 respectively in red and blue bands during the November - December run, indicating relative increase in the abundance of smaller dust particles out ward. Radial brightness variation seen near the nucleus on November 6 is indicative of the presence of a blob or shocked region beyond 10" from the nucleus which has gradually smoothened by December 13. The brightness distribution is found steeper during November 5-7 as compared to on December 13.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Optical polarimetry and photometry of comet 17P/Holmes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Optical polarimetry and photometry of comet 17P/Holmes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical polarimetry and photometry of comet 17P/Holmes will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-149245

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.