Table 1
Sample of disks in this study, based on PAH studies by Habart et al. (2004a) and Geers et al. (2006).
| Target | d (pc) | L* (L⊙) | SpT | M* (M⊙) | log Ṁ (M⊙ yr−1) |  (L⊙) |
FPAH3.3 μm (10−14 W m−2) | IPAH3.3 μm,1pc | Disk typeb | Refc |
|---|---|---|---|---|---|---|---|---|---|---|
| ABAur | 155 | 46 | A0 | 2.4 | −7.0 | 3.5 | <1.0±0.2 | <3.0±0.6 | TD | 2 |
| Elias1/V892Tau | 134 | 129 d | A0 | 2 | — | 7.8 | 0.5±0.1 | 0.87±0.18 | TD | 1 |
| HD 100453 | 104 | 6.2 | A9 | 1.5 | −8.3 | 0.1 | 1.3±0.2 | 1.8±0.3 | TD | 3 |
| HD 100546 | 110 | 23 | B9 | 2.2 | −7 | 2.5 | 2.5±0.5 | 3.8±0.8 | TD | 2 |
| HD 135344 | 136 | 6.2 | F5 | 1.6 | −7.4 | 0.1 | <0.5±0.1 | <1.2±0.2 | TD | 2 |
| HD 139614 | 135 | 5.9 | A9 | 1.5 | −8.1 | 0.1 | <0.5±0.1 | <1.1±0.2 | TD | 3 |
| HD 142527 | 157 | 9.1 | F6 | 2.3 | −7.5 | 0.1 | 1.0±0.6 | 3.1±1.9 | TD | 2 |
| HD 169142 | 114 | 20 | A5 | 2 | −8.7 | 0.56 | 1.0±0.2 | 1.6±0.3 | TD | 2 |
| HD 97048 | 185 | 35 | A0 | 2.4 | −8.2 | 2.1 | 1.3±0.3 | 5.6±1.3 | TD | 2 |
| IRS 48 | 134 | 18 | A0 | 2 | −8.4 | 1.1 | 0.24±0.02 | 0.54±0.04 | TD | 2 |
| SR 21 | 138 | 12 | G3 | 2 | −7.9 | 0.04 | 0.35±0.02 | 0.84±0.05 | TD | 2 |
| SYCha | 181 | 0.73 | M0.5 | 0.8 | −9.4 | 0.0004 | <0.008±0.002 | <0.033±0.006 | TD | 2 |
| TCha | 102 | 1.3 | G8 | 1.2 | −8.4 | 0.01 | <0.25±0.05 | <0.33±0.06 | TD | 2 |
| GWLup | 155 | 0.33 | M1.5 | 0.5 | −9.0 | 0.0008 | <0.024±0.005 | <0.072±0.015 | RD | 5 |
| HD 142666 | 148 | 8.7 | A8 | 1.6 | −7.6 | 0.2 | 0.3±0.2 | 0.83±0.55 | RD | 3 |
| HD 163296 | 101 | 17 | A1 | 2.0 | −7.4 | 1 | <0.2±0.04 | <0.26±0.05 | RD | 5 |
| IMLup | 158 | 2.6 | K5 | 0.9 | −7.9 | 0.009 | <0.19±0.04 | <0.60±0.12 | RD | 5 |
| RULup | 159 | 1.5 | K7 | 0.6 | −7.1 | 0.04 | <0.57±0.11 | <1.8±0.4 | RD | 5 |
| V1121Oph/AS209 | 121 | 1.4 | K5 | 0.8 | −7.3 | 0.04 | 0.12±0.02 | 0.22±0.04 | RD | 5 |
| WaOph6 | 123 | 2.9 | K6 | 0.7 | −6.6 | 0.12 | 0.23±0.02 | 0.44±0.04 | RD | 5 |
| DoAr24E | 136 | 1.6 | K0 | 0.6 | −8.5 | 0.004 | <0.041 ±0.008 | <0.095±0.019 | CD | 4 |
| GQLup | 150 | 0.91 | K5 | 0.6 | −7.4 | 0.03 | <0.054±0.011 | <0.15±0.03 | CD | 4 |
| Haro1-17 | 142 | 0.22 | M7 | 0.1 | −99 | 0 | <0.0045±0.001 | <0.011 ±0.002 | CD | 4 |
| HD 104237/DXCha | 108 | 21 | A4 | 1.8 | −6.4 | 1.5 | <0.5±0.1 | <0.73±0.14 | CD | 3 |
| HD 179218 | 266 | 112 | A0 | 3 | − | 6.8 | 1.7±0.2 | 15±1.8 | CD | 6 |
| Sz73 | 155 | 0.18 | K7 | 0.7 | −8.5 | 0.006 | 0.094±0.02 | 0.28±0.06 | CD | 4 |
| WXCha | 189 | 0.86 | M0 | 0.5 | −6.7 | 0.1 | <0.027±0.006 | <0.12±0.03 | CD | 4 |
Notes. a FUV luminosity, integrated from the stellar spectrum (including accretion luminosity) between 912-2050 Å or 6-13.6 eV (Habing 1968). In Figure 3, LFUV is computed at 150 au radius to obtain the parameter χ, similarly to previous studies. b TD = transition disk, CD = compact disk (<20 au), RD = ring disk (see van der Marel & Mulders 2021). c Reference for stellar properties: (1) Herczeg & Hillenbrand (2014), (2) van der Marel (2023), (3) Grant et al. (2023), (4) Manara et al. (2023), (5) Andrews et al. (2018), (6) Vioque et al. (2018). d Whereas Vioque et al. (2018) reports a luminosity of 1.3 L⊙, the higher luminosity by Herczeg & Hillenbrand (2014) is used here as it is more consistent with the stellar mass, which is independently derived from CO kinematics by Long et al. (2021).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.