Abstract
view Abstract Citations (56) References (10) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The binary central star of the planetary nebula LT-5. Feibelman, W. A. ; Kaler, J. B. Abstract The authors have found with the IUE that the true central star of the giant planetary Longmore-Tritton 5 (339+88°1) is a binary companion to the G5 star SAO 82570. The slope of the energy distribution curve indicates that the star may be one of the hottest known. The Mg II doublet associated with the G star is very strong, consistent with the existence of a close binary companion. Publication: The Astrophysical Journal Pub Date: June 1983 DOI: 10.1086/161065 Bibcode: 1983ApJ...269..592F Keywords: Binary Stars; Hot Stars; Planetary Nebulae; Stellar Spectra; Ultraviolet Spectra; G Stars; Iue; Spectral Energy Distribution; Stellar Evolution; Subdwarf Stars; Astronomy full text sources ADS | data products SIMBAD (1) MAST (1) INES (1)
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