1 Introduction
2 Model assumptions and numerical method
3 DESTINY
3.1 Parameter space
Parameter | Simulated values |
---|---|
Mass ratio (perturber mass / host mass) | 0.3, 0.5, 1.0, 2.0, 5.0, 10.0, 20.0, 50.0 |
Angle of periastron [degrees] | 0, 45, 90 |
Orbital inclination [degrees] | 0, 10, 20, 30, 40, 50, 60, 70, 80, 90, 100, 110, 120, 130, 140, 150, 160, 170, 180 |
Periastron distance [au] | 30, 50, 70, 100, 120, 150, 200, 250, 300, 500, 700, 1000 |
3.2 Structure
3.3 Download and usage of the raw data
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x, y, z positions: x_position, y_position, z_position
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inclination: particle_inclination
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eccentricty: particle_eccentricity
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semimajor axis: particle_semimajoraxis
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longitude of ascending node: particle_loan
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angle of periastron (or argument of periapsis): particle_aop
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true anomaly: particle_true_anomaly
3.4 Graphics options
3.5 Advantages of the database
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higher accuracy,
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larger parameter space,
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better resolution in the outer disk areas,
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free choice of initial disk density distribution,
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more flexibility for the user.