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The ring might also contain most of the Sombrero Galaxy's cold molecular gas, [11] although this is an inference based on observations with low resolution and weak detections. [ 13 ] [ 14 ] Additional observations are needed to confirm that the Sombrero galaxy's molecular gas is constrained to the ring.
The ring structure is so perfect and circular that it has been referred to as "The most perfect ring galaxy". [7] The diameter of the 6 arcsecond inner core of the galaxy is about 17 ± 0.7 kly (5.3 ± 0.2 kpc) while the surrounding ring has an inner 28″ diameter of 75 ± 3 kly (24.8 ± 1.1 kpc) and an outer 45″ diameter of 121 ± 4 kly (39 ...
NASA's James Webb Space Telescope has returned incredible new photos of the Sombrero galaxy, offering a new look at the region. The Sombrero galaxy, named for its resemblance to the Mexican hat ...
The Sombrero galaxy looks entirely different in a new image by the James Webb Space Telescope. Instead of a Mexican hat, it appears more like an archery target.
NGC 5746 is located at a distance of 99 million light years [7] and is seen nearly edge-on, bearing a strong resemblance with the galaxy NGC 4565, that is also seen nearly edge-on. Galaxy NGC 5746, by HST. As with the former, it has a box-shaped bulge that is actually a bar seen from one side [7] and a currently modest star formation activity. [8]
[6] Lindsay-Shapley Ring: Volans: Named after its discoverer, Eric Lindsay, his professor Harlow Shapley, and its nature as a ring galaxy. [citation needed] The ring is the result of collision with another galaxy [citation needed] Little Sombrero Galaxy: Pegasus: Named after its similarity to the Sombrero Galaxy. [citation needed] Malin 1: Coma ...
The galaxy is seen edge-on from Earth. It is sometimes referred to as "the little sombrero", a miniature version of Messier 104 . The star field behind NGC 7814 is known for its density of faint, remote galaxies as can be seen in the image here, in the same vein as the Hubble Deep Field .
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