Quote:
Originally Posted by Paul Haese
That is an interesting colour palette, it all seems to fit quite well without appearing to look fluro like. I like the detail too.
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I thought the “accurate” mapping of the Ha, SII and OIII to their emission line colours helped suggest the difference in hue between NGC3603 and NGC3576 when imaged in LRGB. The spectrographic color corrected stars are a bit of a a bit of a lie however, given only narrow band wavelengths of light were collected (yellow stars come out moslty red when not corrected).