Quote:
Originally Posted by Paul Haese
Thanks Robert for your considered comments. I found one or two images out there in cyber land that sort of hinted at the spiral structure. Some of the commentary suggested it might be a barred spiral, that is caused by a night of high cloud in the mix.
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Yes, NGC55 sure looks more regular in deeper exposures. Not surprising, as it is actually a regularly rotating disk structure (as shown by the rotation velocities of its neutral atomic hydrogen gas).
Low luminosity spiral galaxies are not "pretty things" because they are invariably somewhat chaotic in their structure (rarely do they have very well-defined spiral arms). However, much of this irregularity is confined to the distribution of luminous young stars.
[[ maybe M33 is only "pretty" (= strongly two-armed) because of an interaction with M31 ?!? ]]
Here is the GALEX image (downloaded from GalexView interface), which was made from two filters: the Far Ultraviolet band plus the Near Ultraviolet band.
The older stars are seen in the NUV band, which is displayed as yellow. The recently formed luminous O and B stars are extremely prominent in the FUV band, which is displayed as blue.
(even a small amount of current star formation causes the galex FUV band to detect a lot of light)
Any spiral arms that are currently forming stars will "light up like a floodlight" in the galex FUV band. Older spiral arms won't.
Sometimes, I resort to a bit of defocussing of an image to try to get a handle on the main structures in less regular galaxies like this one. Better still, go to 800 nanometers and longer in the wavelength of observation, so as to get rid of the chaotic dusting of superluminous stars.
Here is a really fun comparison, the galaxy NGC 247 as seen by Galex:
My morphological notes (from multi wavelength images) for NGC 247 say "probably one-armed, possibly barred", which is very typical for a lot of low-luminosity spirals.