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- W3186417758 abstract "The aim of this study is to derive the masses of the central stars (CSPN) for a large sample of the planetary nebulae (PN). These masses, M ∗ , are derived from the observed PN positions in three diagnostic diagrams and their comparison with evolutionary tracks of model PN. Two of the diagrams, namely L Zan ( H ) versus T Zan ( H ) and M v versus R neb , have already been used in numerous studies. The third one, S H β versus S V , has recently been introduced by Górny, Stasińska & Tylenda (1996, hereinafter GST96). Here S H β is the nebular surface brightness in H β and S v is defined as F v /(πθ 2 ), where F v is the stellar flux in the V band and θ is the observed nebular angular radius." @default.
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- W3186417758 date "1997-01-01" @default.
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- W3186417758 title "Masses of the central stars of Planetary Nebulae" @default.
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- W3186417758 doi "https://doi.org/10.1017/s007418090012995x" @default.
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