The L 1157 protostellar outflow imaged with the Submillimeter Array

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201118473e]

Table 3

Clump positions.

Clump	RA	Dec	Molecular tracer^a
	J2000	J2000	SiO	H₂CO	CH₃OH

B0b^*	20:39:05.5	68:01:40	N	Y	N
B0f	20:39:10.9	68:01:40	Y	N	N
B0g	20:39:09.8	68:01:39	Y	Y	N
B0d^*	20:39:07.9	68:01:30	Y	Y	Y
B0h	20:39:10.4	68:01:27	N	Y	Y
B0i	20:39:11.5	68:01:27	Y	N	N
B0j	20:39:07.7	68:01:22	Y	N	N
B1g	20:39:10.3	68:01:13	Y	N	N
B1f⁺	20:39:09.0	68:01:13	N	N	Y
B1a^*	20:39:10.0	68:01:12	Y	Y	Y
B1h	20:39:10.6	68:01:11	Y	N	N
B1c^*	20:39:09.9	68:01:06	Y	N	N

Notes.

^(a)

Detections above 4σ are marked Y, non-detections are marked N.

^(*)

Reported also by Benedettini et al. (2007).

⁽⁺⁾

Reported also by Codella et al. (2009).

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