Rolfe, D.J.; Abbott, T.M.C. and Haswell, C.A.
|Google Scholar:||Look up in Google Scholar|
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.
|Item Type:||Book Chapter|
|Academic Unit/Department:||Science > Physical Sciences
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Astrid Peterkin|
|Date Deposited:||08 Aug 2008 10:59|
|Last Modified:||14 Jan 2016 17:04|
|Share this page:|