The infrared coronal lines of Nova Vulpeculae 1984 No 2

Details The infrared coronal lines of Nova Vulpeculae 1984 No 2 The infrared coronal lines of Nova Vulpeculae 1984 No 2

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aj.....95..172g&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 95, Jan. 1988, p. 172-177. Research supported by the University of Minnesota, NSF, a

Astronomy and Astrophysics

Astronomy

45

Infrared Spectra, Novae, Stellar Coronas, Stellar Mass Ejection, Aluminum, Calcium, Magnesium, Neon, Silicon, Spatial Distribution

Scientific paper

The authors report the discovery of near-infrared line emission from high ionization states of aluminum, silicon, calcium, magnesium, and neon within the ejecta shell of Nova Vulpeculae 1984 No. 2. They argue that the observed states are produced by photoionization, and are in ionization equilibrium with a 6×105K low-density plasma which has been greatly enriched in aluminum, neon, and magnesium relative to the Sun. The spatial distribution of the ejecta shell is also discussed.

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