noirlab_noao-m77 June 30th, 2020
Credit: NOIRLab/NSF/AURA
M77 is a type Sb spiral galaxy in the constellation Cetus. For various reasons, it is much more commonly referred to by its NGC number. NGC1068 is the nearest and brightest example of a type II Seyfert galaxy, showing broad and strong emission lines due to high velocity gas in the galaxy's inner regions. A strong radio source known as Cetus A sits in the nucleus.
Provider: NOIRLab
Image Source: https://noirlab.edu/public/images/noao-m77/
Curator: NSF's NOIRLab, Tucson, AZ, USA
Image Use Policy: Creative Commons Attribution 4.0 International License
Detailed color mapping information coming soon...
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