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The extended dust emission around the nova GK persei
Authors:S M Dougherty  L B F M Waters  M F Bode  D J M Kester  TJ R Bontekoe
Institution:(1) Liverpool John Moores University, UK;(2) University of Amsterdam, The Netherlands;(3) SRON, Groningen, The Netherlands;(4) Liverpool John Moores University, UK;(5) SRON Groningen, The Netherlands
Abstract:We have applied maximum entropy reconstruction methods to the IRAS observations of the nova GK Persei to examine the spatial distribution of the far-IR emission. We have discovered discrete regions of emission in a co-linear structure extending to 17 arcmin on either side of the binary system, supporting a stellar origin for the structure. We postulate that the evolved secondary is the progenitor of the circumbinary envelope.
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