Strong CO+ and N2+ Emission in Comet C/2016 R2 (Pan-STARRS)

被引:42
作者
Cochran, Anita L. [1 ]
McKay, Adam J. [2 ]
机构
[1] Univ Texas Austin, McDonald Observ, Austin, TX 78712 USA
[2] Univ Space Res Assoc, NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
关键词
comets: individual (2016 R2); molecular processes; protoplanetary disks;
D O I
10.3847/2041-8213/aaab57
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on imaging and spectroscopic observations of comet C/2016 R2 (Pan-STARRS) obtained with the 0.8 m and 2.7 m telescopes of McDonald Observatory in 2017 November and December, respectively. The comet was at a heliocentric distance greater than 3 au during both sets of observations. The images showed a well-developed tail with properties that suggested it was an ion tail. The spectra confirmed that we were observing welldeveloped bands of CO+ and N-2(+). The N-2(+) detection was unequivocally cometary and was one of the strongest bands of N-2(+) detected in a comet spectrum. We derived the ratio of these two ions and from that we were able to derive that N-2/CO = 0.15. This is the highest such ratio reported for a comet.
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页数:4
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