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


Table 3

Coordinates of channel count peaks and angular distance to the nearest continuum peak, for the sources with a maximum channel count higher than 9.

Source(a) Channel count peak(b) Cont. peak(c) Δα (d) Δδy(d) Dc (e) PAc (f) db (g) PAj (h)


α (hh:mm:ss) δ (dd:mm:ss) α (ss) δ (ss) ′′ ′′ ′′ ° ′′ ° °
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
L1448-2A 03:25:22.382 30:45:13.31 22.405 13.26 − 0.29 0.05 0.30 − 79 0.90 0.33 135 − 45
L1448-NB2 03:25:36.349 30:45:15.05 36.315 15.15 0.44 − 0.10 0.45 102 1.00 0.45
L1448-C 03:25:38.873 30:44:05.28 38.875 05.33 − 0.03 − 0.05 0.06 − 151 1.12 0.05 − 17 163
IRAS2A1 03:28:55.575 31:14:37.04 55.570 37.07 0.06 − 0.03 0.07 113 0.94 0.07 205 25
SVS13A 03:29:03.748 31:16:03.83 03.756 03.80 − 0.11 0.03 0.11 − 75 0.43 0.26 155 − 25
IRAS4A2 03:29:10.427 31:13:32.12 10.432 32.12 − 0.07 − 0.00 0.07 − 94 0.51 0.13 182 0
IRAS4B 03:29:12.008 31:13:08.04 12.016 08.02 − 0.10 0.02 0.10 − 79 0.52 0.20 167 − 13
SerpM-SMM4b 18:29:56.517 01:13:11.72 56.525 11.58 − 0.13 0.14 0.18 − 43 0.64 0.29 10 145
SerpS-MM18a 18:30:04.121 −02:03:02.58 04.118 02.55 0.05 − 0.03 0.06 116 0.55 0.11 188 8
L1157 20:39:06.268 68:02:15.73 06.269 15.70 − 0.01 0.03 0.03 − 12 0.59 0.06 163 − 17

Notes. (a) Continuum source nearest to channel count peak. (b)J2000 equatorial coordinates of channel count peak obtained from Gaussian fit in Fig. 2. (c) J2000 equatorial coordinates of nearest continuum peak from Maury et al. (2019). The hours, minutes, degrees, and arcminutes are not displayed. They are the same as in Cols. 2 and 3. (d) Equatorial offsets of channel count peak with respect to nearest continuum peak. (e) Angular distance between channel count peak and nearest continuum peak. (f) Position angle of vector going from nearest continuum peak to channel count peak, counted east from north. (g) Beam diameter (HPBW) along PAc. This is an average value for setups S1 and S2. (h)Position angle of the blueshifted and redshifted lobes of the outflow/jet from the CALYPSO survey (Podio et al., in prep.), except for L1448-2A for which we take the tentative detection of Kwon et al. (2019).

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