Table 4.
Periods of the eight photometric variable CP3 stars identified in this study.
| (1) | (2) | (3) |
|---|---|---|
| ID_LAMOST | Pour (d) | Plit (d) |
| J050338.55+234349.5 | 2.99(2) | − |
| J060937.73+235218.0 | 11.44(39) | 9.901513 (a), 11.91(7) (b) |
| J061137.11+254307.8 | 6.2(3) (1) | 6.248527 (a), 6.33(5) (b) |
| J063253.86+034220.3 | 1.14(1) | − |
| J063735.23+210443.6 | 2.34(2) | 2.38192 (a), 2.364(3) (b) |
| J063821.84+110846.7 | 4.47(14) | − |
| J071933.80+145655.7 | 2.25(3) | − |
| J195021.63+411958.5 | 6.7675(4) (1) | 6.757 (c), 6.768 (d) |
Notes. The columns denote: (1) LAMOST identifier. (2) Period derived in this study. (3) Literature period. The corresponding references are indicated in the notes.
References.(a)Armstrong et al. (2016), (b)Balona (2016), (c)Balona (2013), (d)Nielsen et al. (2013).
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