The binary central star of the planetary nebula LT-5

Details The binary central star of the planetary nebula LT-5 The binary central star of the planetary nebula LT-5

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...269..592f&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 269, June 15, 1983, p. 592-595.

Astronomy and Astrophysics

Astrophysics

43

Binary Stars, Hot Stars, Planetary Nebulae, Stellar Spectra, Ultraviolet Spectra, G Stars, Iue, Spectral Energy Distribution, Stellar Evolution, Subdwarf Stars

Scientific paper

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.

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