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Table 1
Overview Spitzer papers of YSOs in star-forming regions.
| Cores to Disks (c2d) | d (pc) | Paper | |
|
|
|||
| Ophiuchus (MIPS) | Padgett et al. (2008) | 120 | VII |
| Serpens | Harvey et al. (2007) | 250−400a | IX |
| Cham II | Alcalá et al. (2008) | 180 | X |
| Lupus I,III,IV | Merín et al. (2008) | 150−200 | XI |
| Perseus | Young et al. (2015) | 250 | XII |
| WTTS (c2d) | Padgett et al. (2006), Cieza et al. (2007), Wahhaj et al. (2010) | − | |
| Disks with holes (c2d) | Merín et al. (2010) | − | |
|
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| Gould Belt (GB) | |||
|
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| IC 5146 | Harvey et al. (2008) | 950 | I |
| Cepheus | Kirk et al. (2009) | 300 | II |
| CrA | Peterson et al. (2011) | 150 | III |
| Lupus V & VI (full) | Spezzi et al. (2011) | 150 | IV |
| Ophiuchus North | Hatchell et al. (2012) | 120 | V |
| Auriga | Broekhoven-Fiene et al. (2014) | 450 | VI |
|
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| Others | |||
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| η Cham (IRAC) | Megeath et al. (2005) | 97 | |
| η Cham (MIPS) | Sicilia-Aguilar et al. (2009) | 97 | |
| Cham I | Luhman et al. (2008) | 160 | |
| Taurus | Rebull et al. (2010), Luhman et al. (2010) | 140 | |
| λ Orionis | Hernández et al. (2010) | 450 | |
| Orion | Megeath et al. (2012) | 450 | |
| FEPS | Carpenter et al. (2008) | − | |
Notes.
(a)
The distance to Serpens is uncertain, but recent VLBA observations put it at 415 pc (Dzib et al. 2011), which has been used in this study.
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