It ’s decidedly looking into my psyche and find me need .
Image credit rating : J.A. Toala & M.A. Guerrero ( IAA - CSIC ) , Y.-H. Chu ( UIUC / ASIAA ) , R.A. Gruendl ( UIUC ) , S. Mazlin , J. Harvey , D. Verschatse & R. Gilbert ( SSRO - South ) and ESA
From the European Space Agency :
The atomic number 10 colours in this image are not just beautiful , they also state us about the nebula ’s composition . The promising blue patches show hug drug - ray expelling , spot by the EPIC cameras on ESA ’s XMM - Newton distance observatory , while the wan red and unripe regions trace the glow from ionised atomic number 1 and oxygen , as experience by the Stars and Shadows Remote Observatory South at the Cerro Tololo Inter - American Observatory .
The intense X - beam emission detected by XMM - Newton is give forth from a star at the inwardness of the nebula . This mavin , a Wolf - Rayet star named HD 56925 , is old , massive and press out incredible amounts of material at a staggering pace : the asterisk loses a mass equivalent to that of the Sun in less than 100 000 yr , in the figure of a wind moving quicker than 1500 kilometer / s.
Having such red inhabitants has influenced NGC 2359 ’s mussy embodiment . The nebula consists of a central bubble hem in by a tangled connection of gaseous filaments , thick channels of dark detritus and bright outbursts , where material tangle up by the stellar wind has collided with the surrounding gas and triggered rippling electric shock waves throughout the region .
The blue patches in this image spotlight the nebula ’s hottest neighborhood : the central bubble and a blowout to its lower left . NGC 2359 ’s gas is thought to reach temperatures grade from several million up to tens of meg of degrees .
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