Table 4
Representative or assumed size of spectral line emission in CALYPSO sources.
| Source | Size(a) | Filter(b) | |
|---|---|---|---|
| (′′) | (au) | (′′) | |
| L1448-2A | 1.0 | 290 | 0.8 |
| L1448-2Ab | 1.0(c) | 290 | – |
| L1448-NA | 1.0 | 290 | 1.2 |
| L1448-NB1 | 1.0(c) | 290 | – |
| L1448-NB2 | 1.0(c) | 290 | – |
| L1448-C | 0.5 | 150 | 0.8 |
| L1448-CS | 0.5(c) | 150 | – |
| IRAS2A1 | 0.35 | 100 | 0.8 |
| SVS13B | 0.5 | 150 | 0.8 |
| SVS13A | 0.3 | 90 | 0.8 |
| IRAS4A1 | 0.35(c) | 100 | – |
| IRAS4A2 | 0.35 | 100 | 0.6 |
| IRAS4B | 0.4 | 120 | 0.8 |
| IRAS4B2 | 0.4(c) | 120 | – |
| IRAM04191 | 2.0 | 280 | 1.0 |
| L1521F | 0.5 | 70 | 1.0 |
| L1527 | 1.0 | 140 | 0.8 |
| SerpM-S68N | 0.5 | 220 | 0.8 |
| SerpM-S68Nb | 0.5(c) | 220 | – |
| SerpM-SMM4a | 0.5(c) | 220 | – |
| SerpM-SMM4b | 0.5 | 220 | 0.8 |
| SerpS-MM18a | 0.5 | 180 | 0.8 |
| SerpS-MM18b | 0.5(c) | 180 | – |
| SerpS-MM22 | 1.0 | 350 | 0.8 |
| L1157 | 0.25 | 90 | 0.8 |
| GF9-2 | 1.0 | 470 | 0.8 |
Notes. (a) Representative size (HPBW) of the spectral line emission. The value corresponds to the level of the dashed line in Figs. D.1–D.15 for the sources shown in these figures. (b) Only the lines that have a peak offset from the continuum peak by less than this value were taken into account to estimate the emission size. (c) Assumed value.
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