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Table 2

Notes on mapped regions for individual sources.

Object Continuum Line Sources Outflows Remarks
on off on off single multiple single multiple

Per01 X X X X
Per02 X X X Xc three sources (3), contam. by Per03 (1,2)
Per03 X Xe X X a binary (1,4)
Per04 X nd nd X X
Per05 X X X X

Per06 X X X? Xc contam. by NGC 1333 IRAS 2A in N-W (5)
Per07 X nd nd X Xc contam. in lines in N-W
Per08 X Xe X X
Per09 X Xe X? X?
Per10 X X X Xc two sources (1,2), dominated by YSO 24 (1,2)

Per11 X Xe X Xc NGC 1333 IRAS4A in N-W (5)
Per12 X nd nd X Xc contam. in lines by NGC 1333 IRAS4A in N-W (5)
Per13 X nd nd X? X?
Per14 X X X? X?
Per15 X X X X

Per16 X nd nd X X
Per17 X? nd nd X Xc? Per18 in S-E, nodded on emission
Per18 X X X Xc? B1-b outflow? (2)
Per19 X X X X
Per20 X Xe X X

Per21 X Xe X? X?
Per22 X Xe X? X?

Notes. Columns 2–5 indicate the location of the continuum at 179 μm and line emission peak of the H2O 212−101 (179.527 μm) transition on the maps (whether on or off-center). Columns 69 provide information about the number of sources and their outflows in the mapped region. Contamination by the outflows driven by sources outside the PACS field of view is mentioned in the last column. Extended emission associated with the targeted sources is denoted by “e”. Non-detections are abbreviated by “nd”, while “c” marks the contamination of the targeted source map by outflows from other sources.

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