PAH emission from nova Cen 1986.

Details PAH emission from nova Cen 1986. PAH emission from nova Cen 1986.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989iaus..135p.101h&link_type=abstract

IAU Symposium No. 135: Interstellar dust: contributed papers, p. 101 - 106

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4

Nova Centauri 1986, Novae: Polycyclic Hydrocarbons, Novae: Spectra

Scientific paper

The authors report the discovery of broad emission features between 3.2 μm and 3.6 μm in the spectrum of Nova Cen 1986 (V842 Cen) some 200 days following outburst and remaining prominent for several months. The general characteristics of these features are similar to those attributed to PAH molecules in other dusty sources, although the relative strengths are different, and these observations provide the first clear evidence for molecular constituents other than graphite particles in the ejecta of novae.

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