Hubble captures NGC 1961

Hubble captures NGC 1961

NASA, European Space Agency, c. Dalcanton (University of Washington), R. Foley (University of California – Santa Cruz); Image processing: c. Cooper (NASA Goddard/Catholic University of America)

Galaxy NGC 1961 reveals its impressive spiral arms in this newly released image from NASA’s Hubble Space Telescope. Shimmering blue regions of bright young stars are scattered in the dusty spiral arms wrapped around the galaxy’s glowing center.

NGC 1961 is an intermediate helical and AGN or Active Galactic NucleiGalaxy type. Intermediate spirals lie between the “banned” and “unbarred” spiral galaxies, which means that they do not have a well-defined strip of stars in their centers. AGN galaxies have very bright centers that often outshine the rest of the galaxy at certain wavelengths of light. It is possible that these galaxies have supermassive black holes In their heart they emit bright jets and winds that shape their development. NGC 1961 is a fairly common type of active galactic nucleus that emits low-energy charged particles.

The data used to create this image came from two proposals. Someone studied the previously unobserved Arp galaxiesThe other looked at the progenitors and eruptions of a variety of supernovae.

NGC 1961 is located 180 million light-years away in the constellation Camelopardalis.

Hubble captures a strange pair of spiral galaxies

the quote: Hubble Captures Galaxy NGC 1961 (2022, September 16) Retrieved September 16, 2022 from

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