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Figure 1:
Phase distribution of the ![]() ![]() |
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Figure 2: y light curve and b-y and u-b colour curves (instrumental system) for AD Boo. |
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Figure 3: y light curve and b-y and u-b colour curves (instrumental system) for HW CMa. |
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Figure 4: y light curve and b-y and u-b colour curves (instrumental system) for SW CMa. |
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Figure 5: Apsidal motion for SW CMa. O-C are the residuals (days) from the linear part of the apsidal motion ephemeris defined by the parameters given in Table 4. The full and dashed curves represent predictions from the apsidal motion parameters for primary (triangles) and secondary (squares) eclipses, respectively. Only the photoelectric observations are shown. |
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Figure 6: y light curve and b-y and u-b colour curves (instrumental system) for V636 Cen. |
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Figure 7:
Apsidal motion for V636 Cen.
O-C are the residuals (days)
from the linear part of the apsidal motion ephemeris defined by the
parameters given in Table 5.
The full and dashed curves represent predictions
from the apsidal motion parameters for primary (triangles)
and secondary (squares) eclipses, respectively. Only the
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Figure 8: y light curve and b-y and u-b colour curves (instrumental system) for VZ Hya. |
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Figure 9: y light curve and b-y and u-b colour curves (instrumental system) for WZ Oph. |
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