A high-resolution infrared spectral survey of Comet C/1999 H1 Lee

被引:46
作者
Dello Russo, Neil [1 ]
Mumma, Michael J.
DiSanti, Michael A.
Magee-Sauer, Karen
Gibb, Erika L.
Bonev, Boncho P.
McLean, I. S.
Xu, Li-Hong
机构
[1] Catholic Univ Amer, Dept Phys, Washington, DC 20064 USA
[2] NASA, Goddard Space Flight Ctr, Solar Syst Explorat Div, Planetary Syst Lab, Greenbelt, MD 20771 USA
[3] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[4] Rowan Univ, Dept Chem & Phys, Glassboro, NJ 08028 USA
[5] Univ Missouri, Dept Phys & Astron, St Louis, MO 63121 USA
[6] Univ Toledo, Dept Phys & Astron, Ritter Astronphys Res Ctr, Toledo, OH 43606 USA
[7] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[8] Univ New Brunswick, Dept Phys Sci, Ctr Laser Atom & Mol Sci, St John, NB E2L 4L5, Canada
基金
美国国家航空航天局; 加拿大自然科学与工程研究理事会;
关键词
comets; infrared; observations; spectroscopy;
D O I
10.1016/j.icarus.2006.04.020
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We obtained high-resolution (lambda/Delta lambda similar to 25,000) spectra of Comet C/1999 H1 (Lee) on UT 1999 August 19.6 and 21.6 using the cross-dispersed Near InfraRed SPECtrometer (NIRSPEC) at the Keck Observatory atop Mauna Kea, HI. Here we present spectra of Comet Lee between 2.874 and 3.701 mu m (3479-2702 cm(-1)) representing the most complete high-resolution infrared survey of a comet to date in this wavelength region. Using published line lists and laboratory spectra we have identified 444 of the 545 distinct emission features present in these spectra. We have tabulated the rest frequencies, assignments, relative intensities, and signal-to-noise ratios of all detected emissions. In addition to gaining insights into the chemistry of Comet Lee, this survey provides a valuable tool for planning future high-resolution infrared observations of comets and other astronomical targets, and for retrospective comparison to existing high-resolution infrared datasets. (c) 2006 Elsevier Inc. All rights reserved.
引用
收藏
页码:255 / 276
页数:22
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