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Hi all,

An image of the nova remnant Cederblad 211, corresponding to the star R Aqr, has been uploaded. This star is a binary system with one of the members being a white dwarf. It pulls material off the primary Mira-type variable star and then explodes as a recurrent nova leaving the beautiful Ced 211 behind… You can find the image and some more info at:

R Aquarii. Cederblad 211


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