Detection of a molecular hydrogen envelope around nova GK Persei
D.P.K. Banerjee, A. Evans, T. Liimets, C.E. Woodward, T.R. Geballe, V. Joshi, S. Starrfield

TL;DR
This paper reports the discovery of a bipolar molecular hydrogen shell around nova GK Persei, indicating complex interactions between nova ejecta and surrounding material, challenging the idea that the nebula is a typical planetary nebula.
Contribution
It provides the first detection of a molecular hydrogen envelope around GK Persei and clarifies its nature as a nova remnant rather than a planetary nebula.
Findings
Detection of a bipolar H2 shell co-spatial with Halpha nebulosity.
H2 emission likely from neutral zone between shocks.
Nebulosity is from ionized pre-existing material, not a planetary nebula.
Abstract
The eruption of Nova Persei 1901 (GK Per) occurred 125 yrs ago; remarkably it still holds major surprises. Using data from the Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer (SPHEREx), we find it has a bipolar molecular hydrogen shell. This shell, which has dimensions 18'x10', is co-spatial with the Halpha nebulosity surrounding the nova, which is purported to be an ancient planetary nebula (PN). The shell is detected most strongly in the 0--0 S(9) 4.6947 micron line. A filament of emission in the S(9) 4.6947 micron line is seen 45" SW of GKPer. This coincides, over much of its length, with the site of X-ray and non-thermal radio emission where the 1901 nova ejecta impinges on the ambient medium. We propose that the H_2 emission from the filament arises from the predicted neutral zone between the forward and reverse shocks. Since it is…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astrophysics and Star Formation Studies · Astronomy and Astrophysical Research
