Nova V 1819 Cygni during diffuse-enhanced and nebular phases

Details Nova V 1819 Cygni during diffuse-enhanced and nebular phases Nova V 1819 Cygni during diffuse-enhanced and nebular phases

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.238p..29a&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 238, May 1, 1989, p. 29P-35P.

Astronomy and Astrophysics

Astronomy

6

Astronomical Spectroscopy, Nebulae, Novae, Astronomical Catalogs, Infrared Astronomy, Light Curve, Ultraviolet Astronomy, Visible Spectrum

Scientific paper

Nova V 1819 Cygni has been observed spectroscopically from 3320 to 10,570 A between days 33 to 44 after maximum light, and in the near IR on days 302 and 398. The measured spectral features are given. The light-curve indicates a distance of about 4.4 kpc. In the diffuse-enhanced phase, the luminosity at maximum visible light is found to be just below the Eddington limit.

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