Differences
This shows you the differences between two versions of the page.
molecules:ism:nh [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:nh [2019/10/18 12:52] (current) – mueller | ||
---|---|---|---|
Line 3: | Line 3: | ||
One and two transitions of the //A// < | One and two transitions of the //A// < | ||
D. M. Meyer and K. C. Roth,\\ | D. M. Meyer and K. C. Roth,\\ | ||
- | **[[http:// | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
The transitions involve an //R//(0) component in both cases as well as a //Q//(0) component of the //v// = 0 – 0 vibrational band system near 335.8 and 335.4 nm, respectively. | The transitions involve an //R//(0) component in both cases as well as a //Q//(0) component of the //v// = 0 – 0 vibrational band system near 335.8 and 335.4 nm, respectively. | ||
Line 9: | Line 9: | ||
The detection of one fine struture component of the //N// = 2 – 1 pure rotational transition toward Sgr B2 was reported by\\ | The detection of one fine struture component of the //N// = 2 – 1 pure rotational transition toward Sgr B2 was reported by\\ | ||
J. Cernicharo, J. R. Goicoechea, and E. Caux,\\ | J. Cernicharo, J. R. Goicoechea, and E. Caux,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
a second fine structure component of that transition was reported in\\ | a second fine structure component of that transition was reported in\\ | ||
J. R. Goicoechea, N. J. Rodríguez-Fernández and J. Cernicharo, | J. R. Goicoechea, N. J. Rodríguez-Fernández and J. Cernicharo, | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
Extended Molecular Absorption, Photodissociation, | Extended Molecular Absorption, Photodissociation, | ||
// | // | ||
Line 19: | Line 19: | ||
A plethora of reports on observations of one or more fine structure components of the //N// = 1 – 0 transition in absorption carried out with // | A plethora of reports on observations of one or more fine structure components of the //N// = 1 – 0 transition in absorption carried out with // | ||
a photon-dominated region: A. Fuente, O. Berné, J. Cernicharo, et al.:\\ | a photon-dominated region: A. Fuente, O. Berné, J. Cernicharo, et al.:\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
a young stellar object: A. O. Benz, S. Bruderer, E. F. van Dishoeck, et al.:\\ | a young stellar object: A. O. Benz, S. Bruderer, E. F. van Dishoeck, et al.:\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
the sight line toward a high-mass star-forminbg region: C. M. Persson, J. H. Black, J. Cernicharo, et al.:\\ | the sight line toward a high-mass star-forminbg region: C. M. Persson, J. H. Black, J. Cernicharo, et al.:\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
and another young stellar object: P. Hily-Blant, S. Maret, A. Bacmann, et al.:\\ | and another young stellar object: P. Hily-Blant, S. Maret, A. Bacmann, et al.:\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
In this context, also ND was observed in two fine structure components of the //N// = 1 – 0 transition by:\\ | In this context, also ND was observed in two fine structure components of the //N// = 1 – 0 transition by:\\ | ||
A. Bacmann, E. Caux, P. Hily-Blant, et al.\\ | A. Bacmann, E. Caux, P. Hily-Blant, et al.\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||