The Extended Dust Emission around the Nova GK Persei

Details The Extended Dust Emission around the Nova GK Persei The Extended Dust Emission around the Nova GK Persei

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..451d&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 451-452

Astronomy and Astrophysics

Astrophysics

Scientific paper

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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