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Re: [APML] Blue in Packman nebula, real or not?
Hi Joe,
I also think that it is real. But I don't attribute it to the H-beta and
OIII lines that some people have suggested. There is also an OII
emission line in the near-UV at 373nm, as well as H-gamma, H-delta and
H-epsilon between ~390-430nm in the violet (which Dean's response
referred to), all of which are registered by colour films on their
blue-sensitive layer. This blue, added to the H-alpha red, is what makes
highly-excited nebulae like M42 look "pink" rather than red, in
unfiltered colour film shots.
If you see photos of M42 taken with a filter which cuts out these UV &
violet lines (eg. a minus-violet, yellow, or deep-sky filter), you'll
notice that the colour is a much purer red - despite the fact that the
H-beta and OIII lines are still transmitted along with the H-alpha.
My experience, using a high performance Astronomiks UHC filter and E200
film on the Orion-Monoceros area, is that it records everything in the
green (H-beta, OIII) and red (H-alpha) channels. Almost nothing is
recorded in the blue channel. This proves that H-beta and OIII register
as "green" on E200, not (or hardly at all) as "blue".
Ray "who finds the Astronomiks UHC to be a wonderful filter; fantastic
visually also in my 120mm f5 RFT achromat" Butler.
Joe & Leslie Schaefer wrote:
> Hi
> I finished processing my images of the Packman nebula and I was
> wondering if anyone knows if this nebula has blue in its core area? The
> image link below is a result of three images (60/90/75 minute
> exposures). Stacked in PW and processed in PS. Did I over process this
> image or is it real?
> Thanks, Joe
>
> www.starfillednights.com/image_data/ngc281_image_data.htm
> <http://www.starfillednights.com/image_data/ngc281_image_data.htm>
>
>
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--
Dr. Ray Butler (ray.butler@nuigalway.ie || ray@physics.nuigalway.ie)
Lecturer, Dept. of Physics || Computational Astrophysics Laboratory
National University of Ireland, Galway, University Road, Galway, Ireland.
Tel: +353-91-524411 ext. 3788 FAX: +353-91-525700
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