Quote:
Originally Posted by Jon
Here are four spectra from 6 December (initial maximum) to 16 December showing the evolution of the lines to I think the level of resolution achievable with my SA100 and system.
Apart from the obvious Balmer emission lines (and hint of P Cygni visible in the 6/12 Ha line profile), and the clear evolution of the FeII lines, there is what I think is NaI at 5889. Also strong growth of an emission line around 7773 - is it the OI triplet?
Cheers
Jonathan
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Looking great Jonathan!
Do you think you will submit them to the ARAS database? Mine are looking awful lonely there, and represent a very low bar to exceed
I'm clouded out again tonight.
I wonder if that feature at ~7770A might be second order contamination, or do you have something in place to cut that?