supernova remnants tagged posts

Webb captures the Spectacular Galactic Merger Arp 220

Webb captures the spectacular galactic merger Arp 220
Credit: IMAGE: NASA, ESA, CSA, STScI, Image processing: Alyssa Pagan (STScI)

Shining like a brilliant beacon amidst a sea of galaxies, Arp 220 lights up the night sky in this view from NASA’s James Webb Space Telescope. Actually two spiral galaxies in the process of merging, Arp 220 glows brightest in infrared light, making it an ideal target for Webb. It is an ultra-luminous infrared galaxy (ULIRG) with a luminosity of more than a trillion suns. In comparison, our Milky Way galaxy has a much more modest luminosity of about ten billion suns.

Located 250 million light-years away in the constellation of Serpens, the Serpent, Arp 220 is the 220th object in Halton Arp’s Atlas of Peculiar Galaxies. It is the nearest ULIRG and the brightest of the three galactic mergers closest to Earth.

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Supernova Simulations reveal how Stellar Explosions Shape Debris Clouds

image of a supernova
A supernova creates a cloud of debris that bears an imprint of the explosion. In this visualization of the simulation data, one quarter of the remnant’s outer shell has been removed to reveal the clumps of matter within (colors denote different materials). Credit: Reproduced from Ref. 1 by permission of the AAS.

Astronomers are now in a better position to interpret observations of supernova remnants thanks to computer simulations of these cataclysmic events by RIKEN astrophysicists.

When certain types of stars die, they go out in a blaze of glory—an incredibly powerful explosion known as a supernova. One of the most common forms of supernova, typeIa, starts with a dense white dwarf star that has burned up its hydrogen fuel...

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