The galaxy NGC 1961 unfurls its attractive spiral arms on this newly launched picture from NASA’s Hubble Area Telescope. Glittering, blue areas of vivid younger stars dot the dusty spiral arms winding across the galaxy’s glowing middle.
NGC 1961 is an intermediate spiral and an AGN, or active galactic nuclei, sort of galaxy. Intermediate spirals are in between “barred” and “unbarred” spiral galaxies, that means they do not have a well-defined bar of stars at their facilities. AGN galaxies have very vivid facilities that usually far outshine the remainder of the galaxy at sure wavelengths of sunshine. These galaxies seemingly have supermassive black holes at their cores churning out vivid jets and winds that form their evolution. NGC 1961 is a reasonably widespread sort of AGN that emits low-energy-charged particles.
The information used to create this picture got here from two proposals. One studied beforehand unobserved Arp galaxies, whereas the opposite regarded on the progenitors and explosions of a wide range of supernovae.
Situated about 180 million light-years away, NGC 1961 resides within the constellation Camelopardalis.
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Hubble captures galaxy NGC 1961 (2022, September 16)
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