Evidence for Dust-related X-Ray Emission from Comet C/1995 O1 (Hale-Bopp)

We report the discovery of X-ray emission from comet C/1995 O1 (Hale-Bopp) bythe LECS instrument on-board BeppoSAX on 1996 September 10--11. The 0.1--2.0keV luminosity decayed by a factor of 2 on a timescale of ~10 hr with a meanvalue of 5.10E16 erg s-1. The spectrum is well fit by a thermal bremsstrahlungmodel with a temperature of 0.29 +/- 0.06 keV, or a power-law with a photonindex of 3.1 +{0.6} -{0.2}. The lack of detected C and O line emission placessevere constraints on many models for cometary X-ray emission, especially thosewhich involve X-ray production in cometary gas. The luminosity is a factor ofat least 3.4 greater than measured by Extreme Ultraviolet Explorer (EUVE) 4days later. This difference may be related to the emergence from the nucleus on1996 September 9 of a dust-rich cloud. Over the next few days the cloudcontinued to expand becoming increasingly tenuous, until it had reached anextent of ~3.10E5 km (or ~2 arcmin) by the start of EUVE observation. Wespeculate that the observed reduction in X-ray intensity is evidence for dustfragmentation. These results support the view that cometary X-ray emissionarises from the interaction between solar X-rays and cometary dust.Comment: 17 pages. 4 postscript figs (2 in color). Accepted for publication in ApJ (Letters