A spectrophotometric study of the nebula around FG SGE

Details A spectrophotometric study of the nebula around FG SGE A spectrophotometric study of the nebula around FG SGE

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....71..102k&link_type=abstract

Astronomy and Astrophysics, vol. 71, no. 1-2, Jan. 1979, p. 102-105. Research supported by the Israel Commission for Basic Rese

Astronomy and Astrophysics

Astrophysics

1

Astronomical Spectroscopy, Planetary Nebulae, Stellar Envelopes, Variable Stars, Emission Spectra, H Lines, Ion Emission, Oxygen Spectra

Scientific paper

Relative intensities of emission lines observed in the nebula PK 60-7.1 deg in the year 1976 are presented. The spectrum shows characteristics of medium or low excitation. Some change in the spectrum as compared to its appearance in 1960 is suspected. The spectrum may be fitted to theoretical models of a nebula in a nonequilibrium state, although by no means uniquely.

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