Spiral Structure in WZ Sagittae around the 2001 Outburst Maximum

Publications of the Astronomical Society of Japan(2002)

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摘要
Intermediate-resolution phase-resolved spectra of WZ Sge were obtained on five consecutive nights (July 23–27) covering the initial stage of the 2001 superoutburst. Double-peaked emission lines of He II at 4686 Å, which were absent on July 23, emerged on July 24 together with emission lines of C III $/$ N III Bowen blend. Analyses of the He II emission lines using the Doppler tomography revealed a...
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关键词
accretion, accretion disks,stars: cataclysmic variables,stars: dwarf novae,stars: individual (WZ Sge)
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