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molecules:ism:co-plus [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:co-plus [2019/10/18 12:48] (current) – mueller | ||
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CO< | CO< | ||
W. B. Latter, C. K. Walker, and P. R. Maloney,\\ | W. B. Latter, C. K. Walker, and P. R. Maloney,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
// | // | ||
The strongest 2 – 1 line was also detected toward the planetary nebula NGC 7027; this is a late type star phase after the AGB (asymptotic giant branch) phase. | The strongest 2 – 1 line was also detected toward the planetary nebula NGC 7027; this is a late type star phase after the AGB (asymptotic giant branch) phase. | ||
Line 9: | Line 9: | ||
The molecular cation has also been seen in the reflection nebula NGC 7023 which is in the vicinity of a Be star:\\ | The molecular cation has also been seen in the reflection nebula NGC 7023 which is in the vicinity of a Be star:\\ | ||
A. Fuente, J. Martin-Pintado, | A. Fuente, J. Martin-Pintado, | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
C. Ceccarelli, E. Caux, M.Wolfire, A. Rudolph, B. Nisini, P. Saraceno, and G.J. White,\\ | C. Ceccarelli, E. Caux, M.Wolfire, A. Rudolph, B. Nisini, P. Saraceno, and G.J. White,\\ | ||
have reported on\\ | have reported on\\ | ||
- | **[[http:// | + | **[[https://ui.adsabs.harvard.edu/ |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
in rather highly excited rotational states (// | in rather highly excited rotational states (// |