Free Access
Table B.1.
Spatially resolved systems.
| Name | Instrument | λ (μm) | a (AU) | Rin (AU) | Rout (AU) | i (°) | PA (°) | Reference |
|---|---|---|---|---|---|---|---|---|
| HD 15115 | LBT/PISCES | 3.8 | (...) | 48 | 96E/120W | 87 | 275 | Rodigas et al. (2012) |
| HD 15115 | HST/STIS | Visible | (...) | ≤19 | 336E/586W | nearly edge-on | 30 | Schneider et al. (2014) |
| HD 15115 | Gemini/NICI | Near IR | 96 | (...) | (...) | 86.2 | 98.5 | Mazoyer et al. (2014) |
| HD 15115 | Subaru/IRCS | 1.63 | (...) | 92 | 337E/589W | 86.3 | 278.63 | Sai et al. (2015) |
| HD 15115 | SMA | 1300 | (...) | 46 | 118 | 87 | 278.5 | MacGregor et al. (2015) |
| HD 30447 | HST/NICMOS | Visible | (...) | 60 | 200 | nearly edge-on | 35 | Soummer et al. (2014) |
| HD 61005 | HST/STIS | Visible | 147 | 38 | 256 | 85.1 | 70.3 | Schneider et al. (2014) |
| HD 61005 | HST/ACS | 0.6 | (...) | ≤33 | 110 | 80.3 | 71.7 | Maness et al. (2009) |
| HD 61005 | HST/NICMOS | 1.1 | (...) | ≤11 | 223 | (...) | 160 | Hines et al. (2007) |
| HD 61005 | SMA | 1300 | 73 | (...) | (...) | 70.3 | 84.3 | Steele et al. (2016) |
| HD 61005 | Herschel | 70, 100, 160 | 96 | 90 | 101 | 67 | 65 | Morales et al. (2016) |
| HD 61005 | VLT/NACO | 1.65 | 65 | 65 | 149 | 84.3 | 70.3 | Buenzli et al. (2010) |
| HD 61005 | VLT/SPHERE, ALMA | Near IR, 1300 | 71 | (...) | (...) | 84.5 | 70.7 | Olofsson et al. (2016) |
| HD 61005 | Gemini/GPI, Keck/NIRC2 | Near IR | 48 | 42 | 121 | 80 | 70.7 | Esposito et al. (2016) |
| HD 71155 | Herschel/PACS | 70, 100 | 69 | (...) | (...) | 56.7 | 167.7 | Booth et al. (2013) |
| HD 95086 | Herschel/PACS | 70, 100, 160 | 202 | 61 | 338 | 25.9 | 98.3 | Moór et al. (2015) |
| β Leo | Herschel/PACS | 100,160 | 39 | 15 | 69 | 35 | 125 | Churcher et al. (2011) |
| HD 106906 | VLT/SPHERE | Near IR | 72 | 72 | 123 | 85 | 104 | Lagrange et al. (2016) |
| HD 106906 | Gemini/GPI | Visible | (...) | 56 | >559 | 85 | 284 | Kalas et al. (2015) |
| HR 4796 | HST/STIS | Visible | 79 | 73 | 86 | 76 | 27 | Schneider et al. (2009) |
| HR 4796 | Gemini/NICI | Near IR | (...) | 71 | 87 | 26 | 26.47 | Wahhaj et al. (2014) |
| HR 4796 | VLT/SPHERE | Near IR | 77 | 73 | 92 | 76.4 | 27 | Milli et al. (2017b) |
| HR 4796 | VLT/NACO | Near IR | 78 | 71 | 84 | 75 | 26.7 | Lagrange et al. (2012) |
| HR 4796 | Keck/MIRLIN | 12.5, 24.5 | 76 | 72 | 87 | (...) | (...) | Wahhaj et al. (2005) |
| HR 4796 | Keck II/OSCIR | 10.8, 18.2 | 76 | 49 | 85 | 77 | 26.8 | Telesco et al. (2000) |
| HR 4796 | HST/NICMOS | Visible | 76 | 65 | 85 | 73.1 | 26.8 | Schneider et al. (1999) |
| HR 4796 | Magellan/MagAO | Near IR | 79 | 74 | 85 | 76.47 | 26.56 | Rodigas et al. (2015) |
| ρ Vir | Herschel/PACS | 70, 100, 160 | 106 | 98 | 114 | 70 | 94 | Morales et al. (2016) |
| HD 131835 | Gemini/TReCS | 11.7, 18.3 | 125 | 41 | 368 | 75 | 61 | Hung et al. (2015b) |
| HD 131835 | Gemini/GPI | Visible | (...) | 89 | 249 | 75.1 | 61.4 | Hung et al. (2015a) |
| HD 131835 | ALMA | 1240 | 120 | 25 | 191 | 73 | 58 | Lieman-Sifry et al. (2016) |
| HD 131835a | VLT/SPHERE | Near IR | 114 | 89 | 166 | 72.6 | −120 | Feldt et al. (2017) |
| HD 141378 | Herschel/PACS | 100, 160 | 202 | 133 | 279 | 62 | 113 | Morales et al. (2016) |
| π Ara | Herschel/PACS | 100, 160 | 122 | (...) | (...) | 40 | 3 | Morales et al. (2016) |
| η Tel | Gemini/TReCS | 11.7, 18.3 | 24 | (...) | (...) | 83 | 8 | Smith et al. (2009) |
| HD 181327 | HST/STIS | Visible | 83 | (...) | (...) | 30.1 | 102 | Schneider et al. (2014) |
| HD 181327 | HST/NICMOS | Visible | 83 | 66 | 100 | 31.7 | 107 | Schneider et al. (2006) |
| HD 181327 | Herschel/PACS | 70, 100, 160 | 84 | 73 | 94 | 31.7 | 107 | Lebreton et al. (2012) |
| HD 181327 | ALMA | 1300 | 81 | 70 | 91 | 30 | 98.9 | Marino et al. (2016) |
| HD 188228 | Herschel/PACS | 70, 100 | 107 | (...) | (...) | 34.3 | 11.4 | Booth et al. (2013) |
| ρ Aql | Herschel/PACS | 100, 160 | 244 | 223 | 265 | 68 | 93 | Morales et al. (2016) |
| HD 202917 | HST/STIS | Visible | 69 | 61 | 76 | 68.6 | 108 | Schneider et al. (2016) |
| HD 202917 | HST/NICMOS | Visible | (...) | (...) | 118 | 70 | 300 | Soummer et al. (2014) |
| HD 206893 | Herschel/PACS | 70 | (...) | 53 | 212 | 40 | 60 | Milli et al. (2017a) |
| HR 8799 | Herschel/PACS | 70, 100, 160, 250 | 218 | 101 | 2000 | 26 | (...) | Matthews et al. (2014a) |
| HR 8799 | ALMA | 1340 | (...) | 149 | 440 | 40 | 51 | Booth et al. (2016) |
| HR 8799 | SMA | 880 | 172 | 152 | 304 | 20 | (...) | Hughes et al. (2011) |
| HR 8799 | Spitzer | 40, 70 | (...) | 92 | 308 | ≤25 | (...) | Su et al. (2009) |
| HR 8799 | CSO | 350 | (...) | 102 | 304 | (...) | (...) | Patience et al. (2011) |
Notes. (a) HD 131835 shows a multiple-rings structure between the belts at ~115 AU and ~6 AU and this could be an indication of the presence of (still forming) planets. Such internal structures, however, are not well constrained and they may be short-living. Therefore, we will treat this system as all the others in the sample noticing that further and more precise analysis could be done, something beyond the aims of this paper.
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.