| |
molecules:ism:hco [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:hco [2019/10/21 17:24] (current) – mueller |
---|
| |
HCO is frequently discussed in conjunction with PDRs (photo dissiciation regions). L. E. Snyder, J. M. Hollis, and B. L. Ulich, reported on the\\ | HCO is frequently discussed in conjunction with PDRs (photo dissiciation regions). L. E. Snyder, J. M. Hollis, and B. L. Ulich, reported on the\\ |
**[[http://cdsads.u-strasbg.fr/abs/1976ApJ...208L..91S|Radio Detection of the Interstellar Formyl Radical]]**\\ | **[[https://ui.adsabs.harvard.edu/abs/1976ApJ...208L..91S|Radio Detection of the Interstellar Formyl Radical]]**\\ |
//Astrophys. J.// **208**, L91–L94 (1976).\\ | //Astrophys. J.// **208**, L91–L94 (1976).\\ |
The NRAO 11 M dish was used to detect the strongest HFS components (//J// = 1.5 – 0.5, //F// = 2 – 1) of the 1<sub>01</sub> – 0<sub>00</sub> transition near 86.671 GHz in emission toward sources showing carbon recombination lines: W3, W51, NGC 2024C, and K3-50. Please note that the NGC 2024 position was stated more precisely in the follwing paragraph. | The NRAO 11 M dish was used to detect the strongest HFS components (//J// = 1.5 – 0.5, //F// = 2 – 1) of the 1<sub>01</sub> – 0<sub>00</sub> transition near 86.671 GHz in emission toward sources showing carbon recombination lines: W3, W51, NGC 2024C, and K3-50. Please note that the NGC 2024 position was stated more precisely in the follwing paragraph. |
J. M. Hollis and E. Churchwell\\ | J. M. Hollis and E. Churchwell\\ |
looked at the\\ | looked at the\\ |
**[[http://cdsads.u-strasbg.fr/abs/1983ApJ...271..170H|Comparison of C<sup>+</sup> Distributions with new Interstellar Sources of HCO Emission]]**\\ | **[[https://ui.adsabs.harvard.edu/abs/1983ApJ...271..170H|Comparison of C<sup>+</sup> Distributions with new Interstellar Sources of HCO Emission]]**\\ |
//Astrophys. J.// **271**, 170–744 (1983).\\ | //Astrophys. J.// **271**, 170–744 (1983).\\ |
The same HFS component was observed with the same instruments as above. New detections were made at a position close to Sgr B2(OH) and in DR21C. | The same HFS component was observed with the same instruments as above. New detections were made at a position close to Sgr B2(OH) and in DR21C. |
L. E. Snyder, M. S. Schenewerk, and J. M. Hollis,\\ | L. E. Snyder, M. S. Schenewerk, and J. M. Hollis,\\ |
reported on the\\ | reported on the\\ |
**[[cdsads.u-strasbg.fr/abs/1985ApJ...298..360S|Observations of Several new Transitions of Interstellar HCO]]**\\ | **[[https://ui.adsabs.harvard.edu/abs/1985ApJ...298..360S|Observations of Several new Transitions of Interstellar HCO]]**\\ |
//Astrophys. J.// **298**, 360–368 (1985).\\ | //Astrophys. J.// **298**, 360–368 (1985).\\ |
Observations of the 2<sub>02</sub> – 1<sub>01</sub> and 3<sub>03</sub> – 2<sub>01</sub> transitions were made. In addition,\\ | Observations of the 2<sub>02</sub> – 1<sub>01</sub> and 3<sub>03</sub> – 2<sub>01</sub> transitions were made. In addition,\\ |
Å Hjalmarson, M. S. Schenewerk, and L. E. Snyder,\\ | Å Hjalmarson, M. S. Schenewerk, and L. E. Snyder,\\ |
reported on\\ | reported on\\ |
**[[cdsads.u-strasbg.fr/abs/1985ApJ...298..360S|Interstellar HCO – Detection of the Missing 3 Millimeter Quartet]]**\\ | **[[https://ui.adsabs.harvard.edu/abs/1985ApJ...298..360S|Interstellar HCO – Detection of the Missing 3 Millimeter Quartet]]**\\ |
//Astrophys. J.// **298**, L71–L74 (1986). | //Astrophys. J.// **298**, L71–L74 (1986). |
| |
H. S. Liszt, J. Pety, M. Gerin, and R. Lucas,\\ | H. S. Liszt, J. Pety, M. Gerin, and R. Lucas,\\ |
detected with the IRAM 30 m telescope\\ | detected with the IRAM 30 m telescope\\ |
**[[http://dx.doi.org/10.1051/0004-6361/201323320|HCO, //c//-C<sub>3</sub>H and CF<sup>+</sup>: three new molecules in diffuse, translucent and “spiral-arm” clouds]]**\\ | **[[https://doi.org/10.1051/0004-6361/201323320|HCO, //c//-C<sub>3</sub>H and CF<sup>+</sup>: three new molecules in diffuse, translucent and “spiral-arm” clouds]]**\\ |
//Astron. Astrophys.// **564**, Art. No. A64 (2014). | //Astron. Astrophys.// **564**, Art. No. A64 (2014). |
| |
M. Agúndez, J. Cernicharo, and M. Guélin\\ | M. Agúndez, J. Cernicharo, and M. Guélin\\ |
in the report on the\\ | in the report on the\\ |
**[[http://dx.doi.org/10.1051/0004-6361/201526317|Discovery of Interstellar Ketenyl (HCCO), a Surprisingly Abundant Radical]]**\\ | **[[https://doi.org/10.1051/0004-6361/201526317|Discovery of Interstellar Ketenyl (HCCO), a Surprisingly Abundant Radical]]**\\ |
//Astron. Astrophys.// **577**, Art. No. L5 (2015). | //Astron. Astrophys.// **577**, Art. No. L5 (2015). |
| |
| |
Contributor(s): H. S. P. Müller; 05, 2015 | Contributor(s): H. S. P. Müller; 05, 2015 |
| |
| |
---- | ---- |
| |
| |