Direct Simulation Monte Carlo Modeling of Ammonia in Comet C/2014 Q2 (Lovejoy)
Ammonia (NH _3 ), likely the most abundant nitrogen-bearing molecule in cometary ices followed by hydrogen cyanide, is believed to be stored in the nucleus predominantly as a parent ice. However, spatial profiles of NH _3 observed in comet C/2014 Q2 (Lovejoy) in the near-infrared region are consiste...
| Hlavní autoři: | , , , , , , , |
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| Médium: | Článek |
| Jazyk: | English |
| Vydáno: |
IOP Publishing
2023-01-01
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| Edice: | The Astronomical Journal |
| Témata: | |
| On-line přístup: | https://doi.org/10.3847/1538-3881/acfee7 |