Quote:
Originally Posted by Merlin66
C II doesn't come up on my data base as significant...
Have a look at the typical nebulae spectrum.
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My mistake, I was looking at 133nm haha
Attached is a table of all of the emission lines from 320nm to 380nm. They’re in angstroms which is nm*10 so the 3444 angstrom OIII line is 344.4nm.
As Ken shows, many of the emission lines aren’t strong but it gives you an indication of how many potentials there are.