Dependence of Chemical Abundance on the Cosmic-Ray Ionization Rate in IC 348
Ions (e.g., ${{\rm{H}}}_{3}^{+}$ , H _2 O ^+ ) have been used extensively to quantify the cosmic-ray ionization rate (CRIR) in diffuse sightlines. However, measurements of the CRIR in low-to-intermediate density gas environments are rare, especially when background stars are absent. In this work, we...
| 出版年: | The Astrophysical Journal |
|---|---|
| 主要な著者: | , , , , , , , , , , |
| フォーマット: | 論文 |
| 言語: | 英語 |
| 出版事項: |
IOP Publishing
2023-01-01
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| 主題: | |
| オンライン・アクセス: | https://doi.org/10.3847/1538-4357/aca657 |
