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- W1982059172 abstract "In enquiring where the lines of high excitation originate in a blue-red binary system, and in seeking the mechanism of variability in those lines, it is desirable to compare times of delay in rise of fluorescence with the time of fluctuation of the stellar stimulus. Equations of Grotrian, Zanstra, and Cillié are therefore employed to correlate rates of growth of fluorescence with certain of the circumstellar conditions, applied to spherical models emitting the Balmer lines and 4686 A., and also the O III and N III fluorescence excited by 304 A. of He II. Data as to observed rates of change, from Swings and Struve, Merrill, Payne-Gaposchkin, McLaughlin, and Sanford, are compared with the suggestions offered by the models. In T Cor B, Z Andr, R Aqar, AX Pers, the comparisons display the contrast between fast-changing inner nebulosity and slow distant relics of previous. outbursts, and facilitate the provisional location of the bright lines in each system. On the other hand, the more steady α Scor and RW Hydr illustrate, from the distance of the M component and its low amplitude of pulsation, the connection suggested by Swings and Struve between binary properties and fluctuations." @default.
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- W1982059172 date "1951-10-01" @default.
- W1982059172 modified "2023-09-26" @default.
- W1982059172 title "Delays in Fluorescence Applicable to the Blue-red Binaries T cor B, Z Andr, R Aqar, Axpers, Scor and Rwhydr" @default.
- W1982059172 doi "https://doi.org/10.1093/mnras/111.5.490" @default.
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