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SNR J0509.5-6731 | by geckzilla
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SNR J0509.5-6731

A supernova remnant with a smooth outer shell in hydrogen emission, and a clumpy inner x-ray shell. The hydrogen emission is shown here in red, while the clumpy x-ray emission is shown in blues, greens, and pinks.

 

I almost didn't finish this, because what I was doing was almost exactly the same as had already been done beautifully, and I try not to redo things. It ended up quite interesting however when I realized there were multiple frames from different years that could be used to show the expansion of the bubble over time. An animation of that is here: flic.kr/p/2heWSpn

 

Hubble proposals used:

The Proper Motion of Supernova Remnant E0509-67.5

Single-Degenerate or Double-Degenerate? The Case for a Third Epoch Observation of the Confirmed Ia Supernova Remnant 0509-67.5

A Search for Surviving Companions of Type Ia Supernovae in the Large Magellanic Cloud

Hubble Heritage 2.0

 

Chandra data:

Red: .10-.70 keV

Green: .70-1.0 keV

Blue: 1.00-5.00 keV

(Obs IDs 776, 7635, 8554)

 

Hubble data:

Red screen: ACS/WFC F658N

Red: WFC3/UVIS F814W

Green: WFC3/UVIS F555W

Blue: WFC3/UVIS F475W

 

North is up.

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Uploaded on September 13, 2019