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| molecules:ism:hono [2019/03/29 15:19] – mueller | molecules:ism:hono [2019/03/29 15:21] (current) – mueller | ||
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| **[[https:// | **[[https:// | ||
| //Astron. Astrophys.// | //Astron. Astrophys.// | ||
| - | 15 lines, mostly between 329.5 and 362.4 GHz with 13 ≤ <i>J</i> & | + | 15 lines, mostly between 329.5 and 362.4 GHz with 13 ≤ //J// ≤ 17 and //K< |
| - | were detected with ALMA in emission toward the Solar-type protostar IRAS 16293–2422 B. The inferred rotational | + | were detected with ALMA in emission toward the Solar-type protostar IRAS 16293−2422 B. The inferred rotational |
| temperature is about 100 K, and the NO/HONO ratio is about 22. | temperature is about 100 K, and the NO/HONO ratio is about 22. | ||