SN 1006

This image of supernova remnant SN 1006 combines data from the Imaging X-ray Polarimetry Explorer (IXPE) and Chandraxray. The red, green and blue elements reflect low, medium and high energy X-rays. The IXPE data, which measure the polarisation of X-ray light, are shown in purple in the upper left corner with the addition of lines representing the outward movement of the magnetic field of the relic.

SN 1006

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WHICH VERY QUICKLY BECOMES BRIGHTER: FU ORIONIS
RARE SPIRAL GALAXIES: UGC 10043

RARE SPIRAL GALAXIES: UGC 10043

ONE OF HUBBLE'S LARGEST MOSAIC IMAGES: 30 DORADUS
EFENDİSİYLE DANS EDEN

EFENDİSİYLE DANS EDEN

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