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Table 3
Comparison of HD 161306 with the confirmed Be binaries showing the effect of radiative interaction.
| Star | Sp. type | v sin i | Ic Hα | FWHM Hα | Orbital per. | K 1 | K 2 | Range | Reference |
| km s-1 | F / F c | Å | d | km s-1 | km s-1 | km s-1 | |||
|
|
|||||||||
| φ Per | B2pe | 450 | 4.0 | 9 | 126.673 | 9.97 | 81.3 | ±120 | Gies et al. (1998) |
| FY CMa | B0.5IVe: | 340 | 1.8 | 11 | 37.253 | 17.4 (14.4) | 128.2 | ±185: | Peters et al. (2008) |
| 59 Cyg | B1-1.5Ve | 450 | 2.0 | 12 | 28.187 | 11.7 | 121.3 | ±180 | Peters et al. (2013) |
| HD 161306 | B0:ne | 160: | 6.2 | 7 | 99.90 | 5: | ±87 | This work | |
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