Nova Cygni 1992 in the post-maximum period

Details Nova Cygni 1992 in the post-maximum period Nova Cygni 1992 in the post-maximum period

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...269l...5a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 269, no. 1-2, p. L5-L8.

Astronomy and Astrophysics

Astrophysics

10

Emission Spectra, Novae, Stellar Magnitude, Stellar Spectrophotometry, Absorption Spectra, Stellar Spectra

Scientific paper

In this letter we describe spectroscopic and photometric observations of Nova Cygni 1992 made in February-April 1992 covering the post-maximum epoch. Nova Cygni 1992 can be identified as a 19.5 mag object on the Palomar Sky Atlas. Its absolute magnitude is estimated to have been about -7.7 mag at maximum and its distance about 1.4 kpc. The strongest emission and absorption lines have been identified and the displacements of P Cygni-type absorption components have been measured. The light curve of this comparatively fast nova is also presented.

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