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First observations of an outbursting comet with the MUSE integral-field spectrograph

机译:MUSE积分场光谱仪对爆发彗星的首次观测

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摘要

We present the first observations of outbursting comet C/2015 ER61 (PANSTARRS) with the Multi-Unit Spectroscopic Explorer (MUSE). The comet was observed on April 9, 2017, only five days after it underwent a significant outburst during which the total brightness increased by a factor of ~7.5. Based on the MUSE observations, we produce simultaneous maps of the CN, C_(2), NH_(2)comae, and the dust coma. In turn, we applied image enhancement techniques in order to reveal features in the coma. By comparing the coma morphology for the dust and CN, C_(2), and NH_(2), we investigate the release mechanism of those gas species in the coma of comet ER61. We present evidence that NH_(2)could be released by icy or organic-rich dust grains.
机译:我们用多单元光谱浏览器(MUSE)展示了C / 2015 ER61彗星(PANSTARRS)的首次观测。彗星于2017年4月9日被观测到,仅在爆发后仅五天,其间总亮度增加了约7.5倍。基于MUSE的观察,我们生成CN,C_(2),NH_(2)彗星和尘埃昏迷的同时图。反过来,我们应用了图像增强技术以揭示昏迷的特征。通过比较尘埃和CN,C_(2)和NH_(2)的彗形形态,我们研究了ER61彗星中这些气体物种的释放机理。我们提供的证据表明,冰冷或富含有机物的尘粒会释放NH_(2)。

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