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| molecules:ism:ho2 [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:ho2 [2019/10/21 17:40] (current) – mueller |
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| B. Parise, P. Bergman, and F. Du,\\ | B. Parise, P. Bergman, and F. Du,\\ |
| used the IRAM 30 m and the APEX 12 m radio telescopes for the\\ | used the IRAM 30 m and the APEX 12 m radio telescopes for the\\ |
| **[[http://dx.doi.org/10.1051/0004-6361/201219379|Detection of the Hydroperoxyl Radical HO<sub>2</sub> toward //ρ// Ophiuchi A: Additional Constraints on the Water Chemical Network]]**\\ | **[[https://doi.org/10.1051/0004-6361/201219379|Detection of the Hydroperoxyl Radical HO<sub>2</sub> toward //ρ// Ophiuchi A: Additional Constraints on the Water Chemical Network]]**\\ |
| //Astron. Astrophys.// **541**, Art. No. L11 (2012).\\ | //Astron. Astrophys.// **541**, Art. No. L11 (2012).\\ |
| The //J<sub>K<sub>a</sub>,K<sub>c</sub></sub>// = 2<sub>0,2</sub> – 1<sub>0,1</sub> and 4<sub>0,4</sub> – 3<sub>0,3</sub> around 130.35 and 260.67 GHz, respectively, were detected. Both transitions displayed fine structure splitting of about 200 MHz. In addition, H-hyperfine splitting was resolved for the lower quantum number transition.\\ | The //J<sub>K<sub>a</sub>,K<sub>c</sub></sub>// = 2<sub>0,2</sub> – 1<sub>0,1</sub> and 4<sub>0,4</sub> – 3<sub>0,3</sub> around 130.35 and 260.67 GHz, respectively, were detected. Both transitions displayed fine structure splitting of about 200 MHz. In addition, H-hyperfine splitting was resolved for the lower quantum number transition.\\ |