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- W1670046029 abstract "The infrared spectrum of what is probably a symbiotic nova showed both the CO absorption lines characteristic of a cool star and a rich emission line spectrum. The hydrogen emission line flux ratios do not agree with case B. If the conditions are however not too far from case B and the lines are formed in a wind from the hot component of the binary, a mass loss rate of about 4 10 −6 M ⊙ yr −1 in 1988 is calculated. Analysis of line profiles shows the presence of two peaks in addition to the main one. This structure is most probably due to bipolar flow. An explanation in terms of an accretion disk created before the outburst is unlikely" @default.
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- W1670046029 date "1991-05-01" @default.
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- W1670046029 title "The infrared spectrum of the eruptive star PU Vulpeculae." @default.
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