JWST Dust NGC7496
Yes, you can use this image! The attribution line is:
NASA / ESA / CSA / Judy Schmidt
Adding a new version of NGC7496 to have the same colorization as NGC628 and IC5332. The center of this galaxy has a very bright point source known as an active galactic nucleus (AGN). You can see it's quite different from the other two which do not have an actively accreting black hole.
Red (screen layer mode): MIRI F2100W
Orange: MIRI F1130W
Cyan: MIRI F770W
Extra overall brightness in grayscale: MIRI F1000W
JWST Dust NGC7496
Yes, you can use this image! The attribution line is:
NASA / ESA / CSA / Judy Schmidt
Adding a new version of NGC7496 to have the same colorization as NGC628 and IC5332. The center of this galaxy has a very bright point source known as an active galactic nucleus (AGN). You can see it's quite different from the other two which do not have an actively accreting black hole.
Red (screen layer mode): MIRI F2100W
Orange: MIRI F1130W
Cyan: MIRI F770W
Extra overall brightness in grayscale: MIRI F1000W