Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/201935428e]


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.1D.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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