Dwarf galaxies can definitely form that way. Take a look at this Hubble image of the Tadpole Galaxy, Arp 188. The blue clumps you can see in the Tadpole's tail are dwarf galaxies in the making:kshiarella wrote:I had the same question as well. Looking closely, there is faint yellow halo around the dense blue (ultraviolet?) core of the object in the lower left. I was guessing that it was an orbiting irregular galaxy. If it is a huge star cluster that has been cast out, is it a possible method of formation of irregular satellite galaxies that they represent a population of stars that were flung from a mother galaxy while in the process of interacting with a third?songwriterz wrote:Looking at the APOD (not the original photo) can anyone tell me what that blue structure is in the lower left corner?
However, I think that the stars in the blue clumps were not so much flung out of the parent galaxy as they were formed in situ out of gas that had been flung out of the parent galaxy. That's what I think about the two prominent blue clumps in today's APOD, too. Particularly the lower left structure is clumpy and irregular enough that I think it is made up of a large gas cloud that has given birth to a lot of stars, but there is still a lot of glowing gas left. So why would this gas cloud look blue and not pink from hydrogen emission? My answer would be that the filters that were chosen for this Hubble image does a relatively poor job at showing the pink emission nebula, so that, in fact, none are visible. But there can be no doubt that the larger galaxy, UGC 1810, does indeed contain pink dots of glowing nebulae. I think that if the Hubble people had imaged UGC 1810 through a hydrogen alpha filter, we would undoubtedly have seen very many pink knots in this galaxy, and I would guess that parts of the lower left blue clump would have been intensely pink.
I'm less certain of the "upper left blue clump". It is smoother and fainter than the other one, and I would guess that it is made up of slightly older and not quite so hot stars. I think it contains vary many stars, compared with the other blue clumps, but the brightest stars are somewhat fainter. This clump could perhaps be regarded as an established and slightly evolved dwarf galaxy.
Ann