Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002em%26p...90..423r&link_type=abstract
Earth, Moon, and Planets, v. 90, Issue 1, p. 423-433 (2002).
Astronomy and Astrophysics
Astronomy
2
Comet C/2001 A2 (Linear), Comets, Dust, Nh2, Polarization
Scientific paper
We present the results of polarimetric and photometricobservations of split Comet C/2001 A2 (LINEAR), which wereobtained at the 70-cm telescope of the Astronomical Observatoryof Kharkiv National University between 30 June and 31 July 2001.The brightest fragment of the comet, nucleus B, was observed.Eight narrowband cometary filters in the continuum and in emissionbands and a wideband red filter have been used. The comet wasobserved through apertures of 88, 33, and 19 arcsec. Polarizationphase curves were obtained for the continuum and for the firsttime, for NH2(0, 7, 0) emission. The degree of polarization ofthe light scattered by the dust decreases with the increase ofaperture size. An important temporal variation of the polarizationwith a rotation of the polarization plane was observed at twophase angles (26.5° and 36.2°). Molecular column densities and production rates of CN, C2,C3, and NH2 species are calculated in the framework of theHaser model. A comparative analysis of the temporal variations ofthe visual magnitudes, gas and dust production rates, dust colorand polarization are presented.
Kiselev Nikolai N.
Rosenbush Vera
Velichko Sergey
No associations
LandOfFree
polarimetric and photometric observations of split comet C/2001 A2 (LINEAR) 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 polarimetric and photometric observations of split comet C/2001 A2 (LINEAR), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and polarimetric and photometric observations of split comet C/2001 A2 (LINEAR) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1893779