This stellar pulsar appears to be the pulsar, in fact, this large star is caused by the shock wave from the explosion.
A recently released image, with three broadcast versions, and a presence in the constellation Mensa, shows dust and gas emanating from the star’s location with the force of the explosion.
“This object – known as DEM L249 – is believed to have been developed by a Type 1a supernova during death spells of a white dwarf,” the Hubble scientists said, “while accumulating could be a case of a binary star system.
This remnant about 160,000 light-years from Earth is relatively nearby and not obscured by much…dust.
The LMC has set up an ideal natural laboratory where astronomers can study the birth, life, and death of stars, as this region is close, oriented toward Earth, on a little bit of light-extending interstellar dust,” the data in this image was collected by Hubble’s Wide Field Camera 3 instrument. , and edited, while editing, 2010, the LMC Systematic about the surviving companions of dwarf stars that have turned into a white supernova.
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