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Sh2-224, Kirby Collins
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Sh2-224

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Sh2-224, Kirby Collins
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Sh2-224

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Sh2-224 is a faint supernova remnant in the constellation Auriga, and is one of 313 H II emission regions cataloged by the astronomer Stewart Sharpless in 1959.   Sh2-224 exhibits not only hydrogen emissions (rendered here in its natural red color), but also has a bit of ionized oxygen (the blue-green arcs).  It is unusual for a supernova remnant...in addition to a more or less spherical shell, it has an additional wing or hat-like structure on one side.  Astronomers thought that this may have been the result of the expanding spherical shock wave hitting a boundary in the surrounding gas, and expanding into a region of much lower density, but recent observations haven't found evidence of this sort of structure in the interstellar medium.  More recent studies proposed that the progenitor (exploding) star was moving at a very high velocity, and the odd structure was a result of interaction with the star's own bow shock.

Interesting paper: https://ui.adsabs.harvard.edu/abs/2019arXiv190908947C/abstract

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Sh2-224, Kirby Collins