Table 7
Stars with known debris discs and planets.
| HIP | HD | Sp Type | [Fe/H] | Ref. | Planet* |
| (dex) | |||||
|
|
|||||
| 522 | 142 | F7V | 0.09b | 9: | gc |
| 1499 | 1461 | G0V | 0.18b | 11 | mlh |
| 7978 | 10647 | F8V | –0.09a | 3 | gc |
| 14954 | 19994 | F8V | 0.19a | 8 | gc |
| 15510 | 20794 | G8V | –0.34a | 10 | mlc |
| 16537 | 22049 | K2V | –0.08a | 1 | gc |
| 27253 | 38529 | G4V | 0.31b | 6 | mgc |
| 27435 | 38858 | G4V | –0.27a | 4 | lc |
| 28767 | 40979 | F8 | 0.13b | 10: | gc |
| 30503 | 45184 | G2V | 0.03 b | 11 | lh |
| 31246 | 46375 | K1IV | 0.23b | 10: | gh |
| 32970 | 50499 | G1V | 0.29b | 10: | gc |
| 33212 | 50554 | F8 | –0.09b | 8 | gc |
| 33719♯ | 52265 | G0V | 0.18b | 8 | gc |
| 40693 | 69830 | K0V | 0.00a | 2 | mlh |
| 42282 | 73526 | G6V | 0.22b | 10: | mgc |
| 47007 | 82943 | G0 | 0.23b | 8 | mgc |
| 58451 | 104067 | K2V | 0.04b | 11 | gc |
| 61028 | 108874 | G5 | 0.17b | 12 | mgc |
| 64924 | 115617 | G5V | 0.00a | 8 | mlh |
| 65721 | 117176 | G5V | –0.03a | 8 | gc |
| 71395 | 128311 | K0 | 0.04a | 8 | mgc |
| 72339 | 130322 | K0V | –0.07b | 12 | gh |
| 94075 | 178911B | G5 | 0.29 b | 10: | gc |
| 97546 | 187085 | G0V | 0.05b | 10: | gc |
| 99711 | 192263 | K2 | –0.01a | 5 | gc |
| 104903 | 202206 | G6V | 0.36b | 10 | mgc |
| 112190 | 215152 | K0 | –0.10c | 11 | mlh |
| 113044 | 216435 | G3IV | 0.24b | 10 | gc |
Notes.
(b) values are set into our metallicity scale as described in Sect. 3.2.
Metallicity for this star is from Sousa et al. (2008) since no value were found in VF05 or NO04.
m = multiplanet system; l = low-mass planet; g = gas giant planet; c = cool planet; h = hot planet (semimajor axis ≤ 0.1 AU, see text).
Spectral type from Montes et al. (2001).
References. (1) Habing et al. (2001); (2) Bryden et al. (2006); (3) Moór et al. (2006); (4) Beichman et al. (2006); (5) Smith et al. (2006); (6) Moro-Martín et al. (2007); (7) Rhee et al. (2007); (8) Trilling et al. (2008); (9) Bryden et al. (2009); (10) Kóspál et al. (2009); (11) Koerner et al. (2010); (12) Dodson-Robinson et al. (2011). The symbol “:” means that non-excess is attributed to the corresponding star in (9) or (10).
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