Nova Serpentis 1983

Details Nova Serpentis 1983 Nova Serpentis 1983

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97.1075s&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Nov. 1985, p. 1075-1077.

Astronomy and Astrophysics

Astronomy

5

Light Curve, Novae, Stellar Spectra, Astronomical Photometry, H Lines, Stellar Magnitude

Scientific paper

A spectrum of Nova Serpentis 1983 has been obtained using the IIDS spectrograph attached to the 2.1-meter telescope at Kitt Peak. A series of 10 spectra were co-added to produce a single spectrum covering the wavelengths in the range 4250-4950 A. The integration time was 300 seconds using an 8.4 arcsec aperture. The photometric and spectroscopic characteristics of the spectrum are discussed in detail. A table listing the spectral line emission intensities of H-beta, H-gamma, and N III in the spectrum of Nova Serpentis 1983 is given, and the photometric light curve is reproduced in graphic form.

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