John,
I have some more information about the strange line of HII regions that is seen in your H-alpha channel.
There is a very strong correspondence between the H-alpha emission found in this part of your image and
a line of blue knots that are seen both in optical images and UV images.
I attach two images of part of NGC 5128;
Firstly, a section of a B+V+I image (displayed as Blue+Green+Red) taken with the ESO 2.2m telescope and the WFI array of CCDs.
(At the ESO website, this is the Public Image with the Identification eso0315a)
Secondly, I attach an Far-Ultraviolet+Near-Ultraviolet composite image taken with the GALEX satellite (using its two available wavelength bands) and downloaded from the GalexView virtual telescope. FUV light is displayed as blue and NUV light is displayed as yellow.
You will note the close correspondence between the blue knots that are seen in the optical image and the Far-ultraviolet emitting knots that are seen in the GALEX image.
Now if I display your image at roughly the same scale and orientation.......
We can easily see that the line of HII regions and the line of blue knots and the line of FUV-emitting knots are exactly the same object or objects!
These objects are most likely bona fide knots of OB stars (and also lower mass stars, at least if they have a typical Initial Mass function)
This is a likely interpretation because the knots are:
- very blue in the optical regime
- very intense in FUV light
and furthermore the stars in the knots are hot enough to ionize the surrounding gas and make it emit in the H-alpha line. Only young and very luminous blue stars are hot enough to produce the ultraviolet photons necessary to make the surrounding gas glow gently in the H-alpha and [OIII] lines.
The knots of recently formed stars are believed to have been formed by an interaction of the plasma jet of N5128 with the surrounding gaseous medium, but I do not believe that this is proven yet. See attached 5GHz radio image of the two jets of N5128 together with the two inner radio lobes.