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The James Webb Space Telescope has captured new detailed portraits of 19 spiral galaxies filled with millions of stars and glowing gas and dust. ‘Mind-blowing’ new images reveal 19 galaxies ...
NGC 4567/8, UGC 7776/7, PGC 42064/9, VV 219, [2] KPG 347, [3] Butterfly Galaxies, [4] Siamese Twin Galaxies, Siamese Twins Galaxies, Siamese Twins [5] [NB 1] NGC 4567 and NGC 4568 (nicknamed the Butterfly Galaxies [ 4 ] or Siamese Twins [ NB 1 ] [ 5 ] ) are a set of unbarred spiral galaxies about 60 million light-years away [ 1 ] in the ...
In response, new research determined [3] NGC 4622's spiral arm sense with a method independent of the previous work. The Fourier component method reveals two new weak arms in the inner disk winding opposite the outer strong clockwise pair. Thus the galaxy must have a pair of arms winding in the opposite direction from most galaxies.
UGC 4457 known as PGC 23935, is a barred spiral galaxy, containing an active galactic nucleus in the Cancer constellation. [1] [2] [3] It is located 500 million light-years away from the Solar System [3] and has a diameter of 290,000 light-years, [1] making it slightly more massive compared to the Milky Way. [4]
NGC 5965 is a spiral galaxy located in the constellation Draco. It is located at a distance of circa 150 million light years from Earth, which, given its apparent dimensions, means that NGC 5965 is about 260,000 light years across. It was discovered by William Herschel on May 5, 1788. [3]
NGC 2207 is in the process of colliding and merging with IC 2163. But unlike the Antennae or the Mice Galaxies, they are still two separate spiral galaxies. They are only in the first step of colliding and merging, with NGC 2207 being in the process of tidally stripping IC 2163. Soon they will collide, probably looking a bit more like the Mice ...
NGC 1024 is a large spiral galaxy of type Sab [1] located in the constellation Aries. Its speed relative to the cosmic microwave background is 3,306 ± 16 km/s, which corresponds to a Hubble distance of 48.8 ± 3.4 Mpc (~159 million light-years). [2] NGC 1024 was discovered by German-British astronomer William Herschel in 1786. [3]
NGC 7496 was one of the first galaxies to be examined by the James Webb Space Telescope, in June 2022, as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS)–JWST survey, whose goal was to study star formation and the interstellar medium in nearby galaxies. [6] The mid infrared images revealed filaments and cavities ...
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