A survey of nova remnants

Details A survey of nova remnants A survey of nova remnants

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.131..467d&link_type=abstract

(IAU, Colloquium on Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments, 93rd, Bamberg, West

Astronomy and Astrophysics

Astrophysics

33

H Alpha Line, Stellar Envelopes, Stellar Spectrophotometry, Supernova Remnants, Astronomical Catalogs, Milky Way Galaxy, Stellar Evolution

Scientific paper

Preliminary results of a survey of exnovae and nova shells are presented, with emphasis on the results of a spectral survey of novae in the southern Milky Way. Continuum magnitudes derived from IDS spectra are accurate to about 0.5 in V and 0.1 in the B-V and V-R colors. The three-dimensional structure for the nebula GK Per, seen in the light of H-alpha, is discussed, and peculiar features of the shell include the missing south-polar cap and the absence of the quarter of the ellipsoid extending from the near center to the west.

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