The Distribution, Excitation and Formation of Cometary Molecules: Methanol, Methyl Cyanide and Ethylene Glycol
Anthony J. Remijan, Stefanie N. Milam, Maria Womack, A. J. Apponi, L., M. Ziurys, Susan Wyckoff, M. F. A'Hearn, Imke de Pater, J. R. Forster, D. N., Friedel, Patrick Palmer, L. E. Snyder, J. M. Veal, L. M. Woodney, and M. C., H. Wright

TL;DR
This study uses interferometric and single-dish observations to analyze the distribution and excitation of organic molecules like methanol, methyl cyanide, and ethylene glycol in comets Hale-Bopp and LINEAR, confirming their origin from the nucleus.
Contribution
It provides detailed measurements of molecular excitation temperatures and production rates, and confirms that these molecules originate from the nucleus rather than the outer coma.
Findings
Methanol excitation temperature ~105 K in Hale-Bopp
Methyl cyanide excitation temperature ~200 K in Hale-Bopp
Methanol production rate ratio ~1.3% in Hale-Bopp
Abstract
We present an interferometric and single dish study of small organic species toward Comets C/1995 O1 (Hale-Bopp) and C/2002 T7 (LINEAR) using the BIMA interferometer at 3 mm and the ARO 12m telescope at 2 mm. For Comet Hale-Bopp, both the single-dish and interferometer observations of CH3OH indicate an excitation temperature of 105+/-5 K and an average production rate ratio Q(CH3OH)/Q(H2O)~1.3% at ~1 AU. Additionally, the aperture synthesis observations of CH3OH suggest a distribution well described by a spherical outflow and no evidence of significant extended emission. Single-dish observations of CH3CN in Comet Hale-Bopp indicate an excitation temperature of 200+/-10 K and a production rate ratio of Q(CH3CN)/Q(H2O)~0.017% at ~1 AU. The non-detection of a previously claimed transition of cometary (CH2OH)2 toward Comet Hale-Bopp with the 12m telescope indicates a compact distribution of…
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