File:SNR J0509 5-6731 (48727564948).png

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Captions

Captions

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.

Summary[edit]

Description
English: 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: https://www.flickr.com/photo.gne?short=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.
Date Taken on 13 September 2019, 13:43:22
Source SNR J0509.5-6731
Author geckzilla
Flickr sets
InfoField
all astronomy; Chandra Processing; Hubble Processing
Flickr tags
InfoField
remnant; expanding; hst; chandra; hydrogen; hubble; clumpy; emission; supernova; shell; bubble; cxo

Licensing[edit]

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This image was originally posted to Flickr by geckzilla at https://flickr.com/photos/54209675@N00/48727564948. It was reviewed on 2 March 2024 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

2 March 2024

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