Four different measures of binary fractions of the anomalously cool giants.
| . | vsini > 10 km s−1 . | 5 < vsini < 10 km s−1 . |
|---|---|---|
| RUWE fbin | 16 ± 8 per cent (5/31) | 23 ± 13 per cent (3/13) |
| Gaia RV fbin | 88 ± 18 per cent (23/26) | 92 ± 27 per cent (12/13) |
| APOGEE fbin | 84 ± 21 per cent (16/19) | 100 ± 33 per cent (9/9) |
| APOGEE fbin, close | 74 ± 20 per cent (14/19) | 100 ± 33 per cent (9/9) |
| . | vsini > 10 km s−1 . | 5 < vsini < 10 km s−1 . |
|---|---|---|
| RUWE fbin | 16 ± 8 per cent (5/31) | 23 ± 13 per cent (3/13) |
| Gaia RV fbin | 88 ± 18 per cent (23/26) | 92 ± 27 per cent (12/13) |
| APOGEE fbin | 84 ± 21 per cent (16/19) | 100 ± 33 per cent (9/9) |
| APOGEE fbin, close | 74 ± 20 per cent (14/19) | 100 ± 33 per cent (9/9) |
Four different measures of binary fractions of the anomalously cool giants.
| . | vsini > 10 km s−1 . | 5 < vsini < 10 km s−1 . |
|---|---|---|
| RUWE fbin | 16 ± 8 per cent (5/31) | 23 ± 13 per cent (3/13) |
| Gaia RV fbin | 88 ± 18 per cent (23/26) | 92 ± 27 per cent (12/13) |
| APOGEE fbin | 84 ± 21 per cent (16/19) | 100 ± 33 per cent (9/9) |
| APOGEE fbin, close | 74 ± 20 per cent (14/19) | 100 ± 33 per cent (9/9) |
| . | vsini > 10 km s−1 . | 5 < vsini < 10 km s−1 . |
|---|---|---|
| RUWE fbin | 16 ± 8 per cent (5/31) | 23 ± 13 per cent (3/13) |
| Gaia RV fbin | 88 ± 18 per cent (23/26) | 92 ± 27 per cent (12/13) |
| APOGEE fbin | 84 ± 21 per cent (16/19) | 100 ± 33 per cent (9/9) |
| APOGEE fbin, close | 74 ± 20 per cent (14/19) | 100 ± 33 per cent (9/9) |
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