Figure 1 shows examples of the periodic wave-like variation in
the UBV LCs for selected symbiotic stars. Table 1 summarizes its
basic characteristics - the amplitude,
,
and the profile
through a parameter a (Sect. 3.2). Photometric UBV observations
used in this paper has been extracted from the literature and are
also referred in Table 1.
![]() |
Figure 1:
Examples of periodic wave-like variation in the LCs of selected
symbiotic binaries. Symbols, |
| Object |
|
|
aU aB aV | Obs. | Note | |
| AXPer | 680 |
|
0.8 0.6 0.5 | 0.6 0.7 0.8 | 1 | |
| BFCyg | 757 |
|
1.1 0.9 0.8 | 0.5 0.6 0.6 | 2 | ss |
| CICyg | 855 |
|
1.2 0.7 0.5 | 0.8 0.8 0.9 | 3 | ss |
| EGAnd | 482 |
|
0.6 0.3 0.2 | 1.0 1.0 1.0 | 4 | sss |
| AGDra | 550 |
|
1.0 0.2 0.1 | 0.5 0.5 0.5 | 5 | |
| V1329Cyg | 958 | 0.18 -0.47 | 1.8 1.3 1.2 | 0.5 0.5 0.5 | 6 | |
| He2-467 | 479 | 0.07 -0.2 | 2.2 0.6 0.3 | 0.6 0.6 1.0 | 7 | s |
| ZAnd | 759 |
|
1.5 1.0 0.7 | 0.5 0.5 0.6 | 8 | ss |
| V443Her | 594 | 0.7 0.4 0.3 | 0.6 0.7 0.8 | 9 | ||
| AGPeg | 813 | 1.1 0.6 0.5 | 0.5 0.5 0.5 | 10 |
Copyright ESO 2001