Located in the Large Magellanic Cloud, the supernova remnant also hides a rapidly spinning neutron star. The mass of this star is around that of the sun or even greater, however, it’s condensed into the area of the city.
The star named DEM L19 or LMC N49, with the trash noticeable in shades of orange and blue, is situated around 160,000 light years from our planet in the heavenly body Dorado.
The picture was made with information from two distinct cosmic examinations utilizing one of Hubble’s resigned instruments – – the Wide Field Planetary Camera 2. The instrument has now been supplanted by the undeniably more impressive Wide Field Camera 3, nonetheless, when it was functional, it conveyed a progression of stunning effort pictures.
The initial two examinations utilized DEM L 190 as a characteristic research center where they concentrated on the cooperation of cosmic explosion remainders and the interstellar medium, the dubious combination of gas and residue that lies between the stars.
The initial two examinations utilized DEM L 190 as a characteristic research facility where they concentrated on the cooperation of cosmic explosion remainders and the interstellar medium, the shaky combination of gas and residue that lies between the stars.
This striking image was created with data from two different astronomical investigations, using one of Hubble’s retired instruments, the Wide Field Planetary Camera 2 (WFPC2). This instrument has since been replaced by the more powerful Wide Field Camera 3 (WFC3), but during its operational lifetime, it contributed to cutting-edge science and produced a series of stunning public outreach images. The first of the two WFPC2 investigations used DEM L 190 as a natural laboratory in which to study the interaction of supernova remnants and the interstellar medium, the tenuous mixture of gas and dust that lies between stars. In the second project, astronomers turned to the Hubble Space Telescope to pinpoint the origin of a Soft Gamma-ray Repeater, an enigmatic object lurking in DEM L 190 which repeatedly emits high-energy bursts of gamma rays.
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