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| molecules:ism:h2o2 [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:h2o2 [2019/10/22 17:09] (current) – mueller |
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| Six rotational transitions of hydrogen peroxide, H<sub>2</sub>O<sub>2</sub>, were searched for with the APEX 12 m radio telescope toward //ρ// Oph A by\\ | Six rotational transitions of hydrogen peroxide, H<sub>2</sub>O<sub>2</sub>, were searched for with the APEX 12 m radio telescope toward //ρ// Oph A by\\ |
| P. Bergman, B. Parise, R. Liseau, B. Larsson, H. Olofsson, K. M. Menten, and R. Güsten,\\ | P. Bergman, B. Parise, R. Liseau, B. Larsson, H. Olofsson, K. M. Menten, and R. Güsten,\\ |
| **[[http://dx.doi.org/10.1051/0004-6361/201117170|Detection of Interstellar Hydrogen Peroxide]]**\\ | **[[https://doi.org/10.1051/0004-6361/201117170|Detection of Interstellar Hydrogen Peroxide]]**\\ |
| //Astron. Astrophys.// **531**, Art. No. L8 (2011).\\ | //Astron. Astrophys.// **531**, Art. No. L8 (2011).\\ |
| The //J<sub>K<sub>a</sub>,K<sub>c</sub></sub>// = 3<sub>0,3</sub> – 2<sub>1,1</sub> and 5<sub>0,5</sub> – 4<sub>1,3</sub> of the //τ// = 4 – 2 ladder near 219.2 and 318.2 GHz, respectively, as well as the 6<sub>1,5</sub> – 5<sub>0,5</sub> and 4<sub>0,4</sub> – 3<sub>1,2</sub> of the //τ// = 2 – 4 ladder near 251.9 and 269.0 GHz, respectively, were detected in emission; albeit the latter one only barely with significance.\\ | The //J<sub>K<sub>a</sub>,K<sub>c</sub></sub>// = 3<sub>0,3</sub> – 2<sub>1,1</sub> and 5<sub>0,5</sub> – 4<sub>1,3</sub> of the //τ// = 4 – 2 ladder near 219.2 and 318.2 GHz, respectively, as well as the 6<sub>1,5</sub> – 5<sub>0,5</sub> and 4<sub>0,4</sub> – 3<sub>1,2</sub> of the //τ// = 2 – 4 ladder near 251.9 and 269.0 GHz, respectively, were detected in emission; albeit the latter one only barely with significance.\\ |
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| Contributor(s): H. S. P. Müller; 06, 2011 | Contributor(s): H. S. P. Müller; 06, 2011 |
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