Table 1
Continuum peak emission at 1.4 mm, detected in Perseus using the CALYPSO survey, where glycolaldehyde emission has been searched for.
| Source | α(J2000)a | δ(J2000)a | Vsys a | d b | F1.4 mm | Lintc | HPB Wsyn | |
| (hms) | (°′″) | (km s-1) | (pc) | (mJy/beam) | (L⊙) | ″×″(°) | ||
|
|
||||||||
| 1.4 mm | 1.3 mm | |||||||
|
|
||||||||
| L1448-2A | 03:25:22.406 | +30 45 13.28 | +4.2 | 232 | 31 | 2.7 | 0 99 × 071 (28°) |
103 × 081 (39°) |
| L1448-NB | 03:25:36.364 | +30 45 14.84 | +4.7 | 232 | 25 | 4.1 | 081 × 067 (67°) |
065 × 048 (48°) |
| L1448-NA | 03 25 36.503 | +30 45 21.87 | +4.7 | 232 | 139 | – | 081 × 067 (67°) |
065 × 048 (48°) |
| L1448-C | 03 25 38.878 | +30 44 05.32 | +5.2 | 232 | 102 | 6.8 | 077 × 063 (22°) |
061 × 038 (33°) |
| IRAS2A3 | 03 28 55.514 | +31 14 34.84 | +7.3 | 235 | 16 | – | 082 × 080 (32°) |
075 × 074 (168°) |
| IRAS2A1 | 03 28 55.575 | +31 14 37.05 | +7.3 | 235 | 99 | 26.7 | 082 × 080 (32°) |
075 × 074 (168°) |
| IRAS2A2 | 03 28 55.677 | +31 14 35.56 | +7.3 | 235 | 12 | – | 082 × 080 (32°) |
075 × 074 (168°) |
| SVS13-B | 03 29 03.075 | +31 15 51.71 | +8.4 | 235 | 122 | 1–2c | 106 × 080 (20°) |
070 × 042 (20°) |
| SVS13-A | 03 29 03.759 | +31 16 03.74 | +8.4 | 235 | 123 | 24.5 | 106 × 080 (20°) |
070 × 042 (20°) |
| IRAS4A2 | 03 29 10.429 | +31 13 32.10 | +7.2 | 235 | 284 | – | 110 × 081 (20°) |
070 × 042 (20°) |
| IRAS4A1 | 03 29 10.531 | +31 13 30.96 | +7.2 | 235 | 795 | 2.8 | 110 × 081 (20°) |
070 × 042 (20°) |
| IRAS4B1 | 03 29 12.012 | +31 13 08.07 | +6.7 | 235 | 449 | 1.0 | 108 × 083 (20°) |
070 × 042 (20°) |
| IRAS4B2 | 03 29 12.840 | +31 13 06.98 | +6.7 | 235 | 53 | – | 108 × 083 (20°) |
070 × 042 (20°) |
Notes.
Positions of the 1.3 mm continuum peak emission and systemic velocities are extracted from the CALYPSO dataset (Codella et al. 2014; Santangelo et al. 2015; Anderl et al. 2016; Maury et al., in prep.).
Internal luminosities were derived from the observed flux at 70 μm (Dunham et al. 2008), a wavelength at which Herschel Gould Belt survey observations (André et al. 2010) provide data at 8″ spatial resolution (see also Ladjelate et al., in prep.). The internal luminosity of SVS13-B is more uncertain due to the proximity to SVS13-A.
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.