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4. Trigonometrical Parallaxes of LB 3303 and LB 3459
Published online by Cambridge University Press: 14 August 2015
Extract
Radcliffe spectra of this star in 1961 confirmed Luyten's suspicion on the basis of colour and proper motion that this object is a bright white dwarf. The profile of Hγ was found to be closely similar to that of o2 Eri B. Hill and Hill have published photometry yielding V = 11.40. The only known white dwarfs brighter than this are Sirius B, o2 Eri B, Procyon B, Feige 34 and CD −38° 10980.
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- Copyright © Reidel 1971
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