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The binary central star of the planetary nebula LT-5Data from the IUE shows that the true central star of the giant planetary Longmore-Tritton 5 (339+88.1 deg) 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.
Document ID
19830056101
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/161065
Authors
Feibelman, W. A. (NASA Goddard Space Flight Center Laboratory for Astronomy and Solar Physics, Greenbelt, MD, United States)
Kaler, J. B. (Illinois, University Urbana, IL, United States)
Date Acquired
August 11, 2013
Publication Date
June 15, 1983
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 269
ISSN: 0004-637X
Subject Category
Astronomy
Report/Patent Number
ISSN: 0004-637X
Accession Number
83A37319
Funding Number(s)
CONTRACT_GRANT: NAG5-171
Distribution Limits
Public
Copyright
Other

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