Astronomy and Astrophysics – Astronomy
Scientific paper
May 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..445a&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, May 1988, p. 445-455. In Russian. In Russian.
Astronomy and Astrophysics
Astronomy
1
Peculiar Stars, Stellar Color, Symbiotic Stars, Ubv Spectra, Electrophotometry, Planetary Nebulae, Stellar Spectrophotometry
Scientific paper
By means of broad and narrow-band photometry in the UBV spectral region the variability of the object He2-467 earlier classified as peculiar central star of a planetary nebula has been revealed. The light amplitude significantly descreases with the wavelength, from 1m.9 in U to 0m.3 in V. The brightness variations were found to be periodic with P = 488 days. The observations of He2-467 were interpreted using the model of a binary consisting of a very hot subdwarf and a G5 II giant. The parameters of both components have been derived. The hot star is probably the evolved low mass nucleus of a planetary nebula already dissipated.
Arkhipova V. P.
Noskova R. I.
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