Quote:
Originally Posted by strongmanmike
Thanks for checking it out guys  Seems that long outer arm is full mostly of new stars then..?
Mike
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Hi Mike,
Yes, indeed....something is making those
new stars in the outer regions of this galaxy, so it must therefore follow that there is
lots of gas and
lots of energy out there, even though there is not much visible in the outermost regions apart from the very faint and unusual arms.
I am certain (at about the 99 percent certainty level) that the outermost arm is experiencing current star formation;
there are usually O and B stars formed in a recent vigorous Star-Formation episode, and these hot young over-luminous stars:
(1) are very prominent in the far-ultraviolet, so they light up like flares in the GALEX satellite images
(2) will light up the gas in the surrounding gas clouds from which they formed, by ionizing the gas and making it glow in Ha, as it requires short wavelength ultraviolet photons from massive luminous new stars to produce an HII region.
One interesting question is, "why should stars form so vigorously, so far from the main optically-bright body of NGC 1512?"
Something has to give interstellar gas a really hard "hit or shock" in order to get it to contract and to form new stars.
So a strong shock wave is required in the outer regions of this galaxy, and also a supply of interstellar gas is needed in order to make the new stars.
It has got me speculating as to whether an encounter with the little companion galaxy might be responsible for the unusual pattern of the outer arms; but the mass difference between the primary and secondary galaxy must be significant. You really need a lot of gas and a lot of energy to make the very-luminous "new & blue" stars that are evident in the outermost arm.
Here is the Galex far-ultraviolet plus near-ultraviolet image, using the GalexView interface. FUV displays as blue, and it is almost certain that the bright knotty FUV emission of the outer arms is coming from newly-formed "hot & young" very-luminous stars.