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À propos de : Imaging and spectroscopy of comet C/2001 Q4 (NEAT) at 8.6 AU from the Sun        

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  • Imaging and spectroscopy of comet C/2001 Q4 (NEAT) at 8.6 AU from the Sun
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  • Comet C/2001 Q4 (NEAT) was observed inbound at an heliocentric distance of 8.6 AU. Broadband filter images in the visible and long slit spectroscopy in the 3500-7000 Å range was recorded. No sign of CN emission was detected and an upper limit for CN production rate of  $1.4\times10^{25}$ molecules s -1 is estimated. The color of the dust in the inner coma is very red with a spectral index of 29%/1000 Å. The radial profile of the dust coma displays steep gradients of 1.7 (inner part) to 2.4 (outer part). The afρ  value, a proxy for the dust production, is measured to be 1500 cm. The coma shows a weak and short conic structure in the northern hemisphere that is interpreted as dust fan produced by an active region on the nuclear surface.
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  • aaek203
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  • © ESO, 2003
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