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| - | ISM/CSS\\ | ||
| - | extragalactic molecules | ||
| - | **Note:** Deuterium isotopic species are given separately only if their method of detection is intrinsically different from that of pure hydrogen ones. We plan to modify this in the future to include them with all hydrogen species. | ||
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| - | The documentations generally provide information on the detection of the respective molecules, including minor isotopic species, molecules in excited vibrational states, or different media in which the species has been detected as well as links to articles. | ||
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| - | All molecules have been detected (a | ||
| - | lso) by rotational spectroscopy in the radiofrequency to far-infrared regions unless indicated otherwise. | ||
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| - | %%*%% indicates molecules that have been detected by their rotation-vibration spectrum,\\ | ||
| - | %%**%%those detected by electronic spectroscopy only. | ||
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| - | **Transition metal molecules** detected in atmospheres of stars by electronic spectroscopy are currently not included. We plan to create a new table in the not so distant future dealing with molecules in stellar atmospheres. In this context, the table of molecules detected in the interstellar medium (ISM) or circumstellar envelopes (CSE) of late type stars, will be split. In the case of some metal monoxides, emission features have been detected in optical or IR spectra. Most likely, this emission indicates a presence of these [[wiki: | ||
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| - | ^2 atoms ^3 atoms ^4 atoms ^5 atoms ^6 atoms ^7 atoms ^8 atoms ^9 atoms ^10 atoms ^11 atoms ^12 atoms ^>12 atoms ^ | ||
| - | | H< | ||