Table 3.
Fraction of long Blazhko periods.
| Ntot | NL | RL | Pop. | Data | Source |
|---|---|---|---|---|---|
| 3141 | 871 | 0.384 | Bulge | OGLE | [1] |
| 641 | 237 | 0.587 | Field | SuperWASP | [2] |
| 310 | 98 | 0.462 | Field | literature | [3] |
| 731 | 258 | 0.545 | LMC | MACHO | [4] |
| 82 | 31 | 0.608 | M3 | literature | [5] |
| 514 | 36 | 0.075 | Field | K2 | [6] |
| 24 | 4 | 0.200 | Field | Kepler | [6] |
Notes. Ntot is the total number of Blazhko stars; NL is the number of stars with PBL > 100 d; RL = NL/(Ntot − NL); [1] = Skarka et al. (2020), [2] = Greer et al. (2017), [3] = the BlaSGalF site by Marek Skarka: https://www.physics.muni.cz/~blasgalf/, [4] = Alcock et al. (2003), [5] = Jurcsik (2019), [6] = this paper. See text for additional notes on the items in this table.
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