The infrared spectrum of comet Hale-Bopp as seen by the Infrared Space Observatory

被引：8
|
作者：
Leech, K [1 ]
Crovisier, J
Bockelée-Morvan, D
Brooke, TY
Hanner, MS
Altieri, B
Keller, HU
Lellouch, E
Lim, T
机构：
[1] ESA, Div Astrophys, ISO Sci Operat Ctr, Villafranca, Spain
[2] Observ Paris Meudon, F-92195 Meudon, France
[3] CALTECH, Jet Prop Lab, Pasadena, CA USA
[4] Max Planck Inst Aeron, Katlenburg Lindau, Germany
[5] Univ London Queen Mary & Westfield Coll, London E1 4NS, England
来源：
EARTH MOON AND PLANETS | 1997年 / 78卷 / 1-3期
关键词：
C/1995; O1; Hale-Bopp; comets; infrared spectroscopy; ISO;
D O I：
10.1023/A:1006283614308
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Spectra of comet C/1995 O1 (Hale-Bopp) were obtained with the Infrared Space Observatory (ISO) at medium resolution with the grating spectrometer in the photometer (PHT-S) and/or at high resolution with the short wavelength spectrometer (SWS) and long wavelength spectrometer (LWS) in April 1996 (Crovisier et al., 1996), September–October 1996 (Crovisier et al., 1997a, b) and December 1997, at distances from the Sun of 4.6, 2.9 and 3.9 AU, respectively. For the first time, high-resolution spectra of a comet covering the entire 2.4 to 200 μm spectral range were obtained.
引用
收藏
页码：81 / 83
页数：3
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