molecules:ism:hco

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

molecules:ism:hco [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:hco [2019/10/21 17:24] (current) – mueller
Line 2: Line 2:
  
 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.
Line 8: Line 8:
 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.
Line 14: Line 14:
 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).
  
Line 30: Line 30:
 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).
  
Line 37: Line 37:
  
 Contributor(s): H. S. P. Müller; 05, 2015 Contributor(s): H. S. P. Müller; 05, 2015
- 
  
 ---- ----
  
  
  • molecules/ism/hco.1551130723.txt.gz
  • Last modified: 2019/02/25 22:38
  • by 127.0.0.1