NASA NTRS · 19750062743
The very slow nova He 3-558
Abstract
The 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.
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Henize, K. G., Liller, W.. 1975-09-15. The very slow nova He 3-558. https://ntrs.nasa.gov/citations/19750062743
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