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The very slow nova He 3-558The emission-line object He 3-558 has been found to be a very slow nova which rose to maximum brightness in 1948 and is probably still fading. Its spectrum and light curve are described, and a distance of 3.5 kpc is derived. No sign of an earlier outburst was found in the Harvard collection of photographs.
Document ID
19750062743
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/153839
Authors
Henize, K. G. (NASA Johnson Space Center Houston, Tex., United States)
Liller, W.
Date Acquired
August 8, 2013
Publication Date
September 15, 1975
Publication Information
Publication: Astrophysical Journal
Volume: 200
Subject Category
Astrophysics
Accession Number
75A46815
Funding Number(s)
CONTRACT_GRANT: NSF GP-40834X
Distribution Limits
Public
Copyright
Other

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