The 2005 encounter
3295 test
particles
Path of secondary: 2005.19-2005.29
The Lehto & Valtonen model predicted that the 2005 encounter
would be at low velocity and distant
from the centre of the accretion disk.
üA long delay from
plane-crossing to optical flare.
üA rather poorly
defined maximum due to the encounter
geometry.
üA large
advance in the date of the optical
flare.
