Nova Aquilae 1982 - A short report

Details Nova Aquilae 1982 - A short report Nova Aquilae 1982 - A short report

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211p...7s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Nov. 1, 1984, p. 7P-13P.

Other

43

Interstellar Extinction, Iue, Novae, Stellar Mass Ejection, Abundance, Binary Stars, Electron Density (Concentration), Electron Energy, Telescopes, Thermonuclear Reactions, White Dwarf Stars

Scientific paper

Observations of Nova Aquilae 1982, obtained using the IUE satellite and the Anglo-Australian telescope, are reported. The nova was unusual in having very high expansion velocities (up to 10000 km s-1), high abundances of heavier elements and large fluxes (reported by other observers) at IR and radio wavelengths. The ejecta had comparable masses in gas and dust, and grain formation may have led to gas-phase element depletions. The hydrogen mass fraction for the ejecta is estimated to be about 0.03. The progenitor may have been a close-binary system.

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