Differences
This shows you the differences between two versions of the page.
Both sides previous revision Previous revision | |||
molecules:ism:hono [2019/03/29 15:20] – mueller | molecules:ism:hono [2019/03/29 15:21] (current) – mueller | ||
---|---|---|---|
Line 7: | Line 7: | ||
**[[https:// | **[[https:// | ||
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
- | 15 lines, mostly between 329.5 and 362.4 GHz with 13 ≤ //J// ≤ 17 and // | + | 15 lines, mostly between 329.5 and 362.4 GHz with 13 ≤ //J// ≤ 17 and // |
- | 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. | ||