|
|
Phase light curves of young binary systems
Phase light curves of binary model that consists of a primary component with mass M1 and a secondary component with mass M2. The binary
is embedded in a circumbinary gas-dust disk whose matter is accreted onto the binary components. The input parameters of the problem are
the accretion rate onto the binary components ( ), the component mass ratio q = M2/M1, the orbital inclination to the line of sight θ,
the eccentricity e, the rotation angle of the apsidal line relative to the observer φ, and the parameter c characterizing viscosity.
The rotation angle of the apsidal line relative to the observer and through "_" the orbit inclination to the line of sight are indicated
in the lower left corner of each diagram.
Model 1: q = M2 : M1 = 0.5, e = 0.5, "hot" disk (с = 0.08), accretion rate = 10-10  /year.
|
|
Model 2: q = M2 : M1 = 0.5, e = 0.5, "warm" disk (с = 0.05), accretion rate = 3 · 10-11 /year. |
|
Model 3: q = M2 : M1 = 0.3, e = 0.5, "warm" disk (с = 0.05), accretion rate = 10-10 /year. |
|
Model 4: q = M2 : M1 = 0.3, e = 0.7, "warm" disk (с = 0.05), accretion rate = 3 · 10-11 /year. |
|
Model 5: q = M2 : M1 = 0.2, e = 0.5, "warm" disk (с = 0.05), accretion rate = 10-10 /year. |
|
Model 6: q = M2 : M1 = 0.1, e = 0.5, "warm" disk (с = 0.05), accretion rate = 3 · 10-10 /year. |
|
Model 7: q = M2 : M1 = 0.1, e = 0.3, "warm" disk (с = 0.05), accretion rate = 10-9 /year. |
|
Model 8: q = M2 : M1 = 0.3, e = 0.1, "warm" disk (с = 0.05), accretion rate = 3 · 10-10 /year. |
|
Model 9: q = M2 : M1 = 0.03, e = 0.5, "warm" disk (с = 0.05), accretion rate = 10-9 /year. |
|
Model 10: q = M2 : M1 = 0.01, e = 0.5, "warm" disk (с = 0.05), accretion rate = 10-9 /year. |
|
|
|
