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Rolfe, Daniel J.; Haswell, Carole A. and Patterson, Joseph
(2001).
DOI: https://doi.org/10.1046/j.1365-8711.2001.04248.x
Abstract
We use the hotspot eclipse times of the newly discovered deeply eclipsing dwarf nova IY UMa to trace out the shape of its disc during the late superhump era. We find an eccentric disc. We show that the brightness of the stream–disc impact region varies as expected with |ΔV|2, where ΔV is the relative velocity of the stream with respect to the velocity of the disc at the impact point. We conclude that the hotspot is the source of late superhump light.
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- Item ORO ID
- 4248
- Item Type
- Journal Item
- ISSN
- 1365-2966
- Keywords
- accretion; accretion discs; binaries: close; binaries: eclipsing; stars: dwarf novae; stars: individual: IY UMa; novae cataclysmic variables
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Depositing User
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