Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.256p..59b&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 256, no. 4, June 15, 1992, p. 59P-63P. Research support
Astronomy and Astrophysics
Astronomy
7
Nebulae, Novae, Stellar Envelopes, Stellar Spectrophotometry, Symbiotic Stars, Cataclysmic Variables, Emission Spectra, H Alpha Line, Line Spectra
Scientific paper
The discovery of an extended nebula of diameter about 24 arcsec around the symbiotic nova V 1016 Cyg from long-slit high-resolution spectroscopy of the H-alpha, He II 468.6-nm and forbidden O III 500.7-nm emission lines is reported. The existence of the nebula is confirmed by CCD images obtained in forbidden O III. The nebula was mapped spectroscopically but the profile changes are difficult to explain in simple terms. The extent of the nebulosity is similar to that inferred for a cool dust component by IRAS observations, for a distance of 0.6 kpc.
Bang M. K.
Bode Michael F.
Ivison Rob J.
Meaburn John
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