Quote:
Originally Posted by Placidus
Fred, your depth of SII is spectacular. Our shot is in NII, not SII.
I've tried hard to get a handle on where you'd see the one and not the other. Both are forbidden transitions, meaning they are only seen in extremely attenuated gas. Both require hard UV (or, perhaps and not relevant here, shock energy) to excite them, so they both need OB stars around. But nitrogen is produced earlier in nucleosynthesis than sulfur, so there might be more NII around in the absence of supernovas to dredge up really deep stuff. Having said that, the similarity between your SII and our NII distribution is very, very close. Almost exact. I think that's reassuring for both of us.
Superb result, Fred.
Best,
Mike and Trish
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Thanks Mike n Trish.
Makes me wonder then that I should always look for NII whenever I cant find SII , just in case,as a substitute.
Did you find NII brighter than SII on Thor?.