KPD 0005 + 5106 - A post-PG 1159 type object?
1985; IOP Publishing; Volume: 290; Linguagem: Inglês
10.1086/162987
ISSN1538-4357
AutoresR. A. Downes, James Liebert, B. Margon,
Tópico(s)Astrophysics and Star Formation Studies
Resumoview Abstract Citations (25) References (14) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS KPD 0005+5106 : a post-PG 1159 type object ? Downes, R. A. ; Liebert, J. ; Margon, B. Abstract In a survey for galactic plane UV-excess objects, a very hot (T about 100,000 K) helium-rich white dwarf is discovered. The object is spectroscopically similar to the pulsating PG 1159 class of stars, with narrow emission lines of He II, probably C IV, and possibly C III/N III, although there is no trace of carbon absorptions. Not all features have positive identifications. This object appears to be an old PG 1159 star, having ceased pulsations during evolution toward a more typical DO white dwarf. Publication: The Astrophysical Journal Pub Date: March 1985 DOI: 10.1086/162987 Bibcode: 1985ApJ...290..321D Keywords: Hot Stars; Milky Way Galaxy; Stellar Evolution; Stellar Spectrophotometry; Ultraviolet Spectra; White Dwarf Stars; Emission Spectra; Helium; Iue; Line Spectra; Spectral Energy Distribution; Spectral Resolution; Astrophysics full text sources ADS | data products SIMBAD (2) MAST (1) INES (1)
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