Table 4
List of known YSOs and late-type stars detected at 18 μm.
| Name | IRC ID | F obs,9 | F obs,18 | KS−[9] | KS−[18] | Spectral | Stellar | Ref. |
| (Jy) | (Jy) | (mag) | (mag) | type | type | |||
|
|
||||||||
| HD 2326 | 0027064–063616 | 99.943 ± 0.725 | 58.287 ± 0.641 | 0.86 | 1.95 | M7 | O-rich AGB | 8 |
| HD 23937 | 0348475–070053 | 37.028 ± 0.144 | 13.536 ± 0.217 | 0.47 | 1.05 | M3 | O-rich AGB | 9 |
| HD 37258 | 0536592–060916 | 1.749 ± 0.004 | 1.622 ± 0.046 | 3.92 | 5.53 | A2V | Herbig Ae | 2 |
| HD 37357 | 0537471–064230 | 1.513 ± 0.001 | 1.671 ± 0.060 | 3.44 | 5.23 | A0e | Herbig Ae | 2 |
| HD 38238 | 0544187+000840 | 1.221 ± 0.004 | 1.690 ± 0.059 | 2.69 | 4.72 | A7IIIe | Herbig Ae | 3 |
| HD 68695 | 0811445–440508 | 0.722 ± 0.010 | 1.275 ± 0.061 | 3.35 | 5.65 | A0V | Herbig Ae | 4 |
| HD 100453 | 1133055–541928 | 5.518 ± 0.077 | 18.744 ± 0.248 | 3.08 | 6.08 | A9Ve | Herbig Ae | 2 |
| HD 107439 | 1221125–491240 | 4.724 ± 0.422 | 3.556 ± 0.132 | 4.07 | 5.44 | G4Vp | post-AGB | 6 |
| HD 120806 | 1351516–034033 | 58.500 ± 0.627 | 29.671 ± 0.085 | 0.97 | 1.91 | M | O-rich AGB | 8 |
| HD 135344 | 1515484–370915 | 1.727 ± 0.063 | 3.285 ± 0.114 | 2.06 | 4.44 | A0V | Herbig Ae | 2 |
| HD 139614 | 1540463–422953 | 2.386 ± 0.057 | 10.568 ± 0.118 | 3.32 | 6.61 | A7Ve | Herbig Ae | 1 |
| HD 142666 | 1556400–220140 | 5.152 ± 0.355 | 6.578 ± 0.007 | 3.48 | 5.42 | A8Ve | Herbig Ae | 2 |
| HD 144432 | 1606579–274310 | – | 7.326 ± 0.259 | – | 5.35 | A9/F0V | Herbig Ae | 2 |
| HD 152404 | 1654448–365318 | 2.032 ± 0.025 | 2.870 ± 0.029 | 2.90 | 4.95 | F5Ve | T Tauri | 2 |
| HD 155555 | 1717255–665704 | 0.816 ± 0.025 | 0.282 ± 0.027 | 0.11 | 0.63 | G7IV | T Tauri | 7 |
| HD 157045 | 1727235–711715 | 80.030 ± 0.106 | 85.198 ± 0.310 | 3.18 | 4.92 | M3III | O-rich AGB | 10 |
| HD 158643 | 1731250–235745 | – | 9.241 ± 0.111 | – | 4.01 | A0V | Herbig Ae | 1 |
| HD 223075 | 2346235+032912 | 174.197 ± 4.056 | 44.205 ± 0.808 | 0.72 | 0.91 | CII | Carbon Star | 5 |
References. (1) Montesinos et al. (2009); (2) Acke et al. (2009); (3) Hernández et al. (2005); (4) Manoj et al. (2006); (5) Abia et al. (2009); (6) Gielen et al. (2008); (7) Schütz et al. (2009); (8) Winters et al. (2003); (9) Sloan & Price (1998); (10) Josselin et al. (1998).
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