Copy the page URI to the clipboard
Rolfe, D.J.; Abbott, T.M.C. and Haswell, C.A.
(2001).
URL: http://books.google.co.uk/books?id=9h2AOyACvU4C&pr...
Abstract
Quiescent Doppler tomography of the newly discovered deeply-eclipsing SU UMa system IY UMa reveals properties of the region where the accretion stream from the donor impacts the edge of the disc. A very strong bright spot is produced and the Keplerian disc emission in the impact region is disrupted or obscured. The differing properties of Hα, Hβ and He I emission will allow physical parameters of the converging flow region to be studied.
Viewing alternatives
Item Actions
Export
About
- Item ORO ID
- 11290
- Item Type
- Book Section
- ISBN
- 3-540-42213-7, 978-3-540-42213-6
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Depositing User
- Astrid Peterkin