Next: Disc Structure
Up: summary
Previous: summary
Paramters adopted in this simulation aregiven below.
For simplicity, the disc is assumed to be isothermal and
Shakura-Sunyaev's viscosity prescription is adopted.
The origin is at the centre of mass of the system,
the semimajor axis is on the
-axis, and
the orbital plane is on the
-plane.
At
the neutron star is at apastron (Phase
0.5).
Stellar parameters |
Mass of the Be star  |
Radius of the Be star  |
Disk temperature
 |
Disk thickness
 |
Sound speed
 |
Break-up velocity
 |
Orbital parameters |
Orbital period
(
) |
Orbital eccentricity  |
Mass ratio (
) |
Semimajor axis
 |
Initial tilt angles: about -axis &
about -axis |
Simulation parameters |
Unit of time (
) |
Unit of length
 |
&
 |
( )
( )
(
) |
( )
( ) |
|
Next: Disc Structure
Up: summary
Previous: summary
Atsuo Okazaki
2002-01-28