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Table 1

Target outflows and central positions for offset calculation.

Source α(J2000) δ(J2000) VLSR Tbola Vel.
(km s-1) (K) Ref.

N1333I2 032855.6 + 311437 7.5 53 (1)
N1333I3 032903.8 + 311604 7.5 136 (1)
N1333I4A 032910.5 + 311331 7.2 34 (1)
HH211 034356.8 + 320050 9.1 30 (1)
IRAS04166 041942.6 + 271338 6.7 56 (2)
L1551 043134.1 + 180805 6.8 106 (1)
L1527 043953.9 + 260310 5.9 42 (1)
HH1-2 053622.8 − 064607 9.4 (3)
HH212 054351.4 − 010253 1.6 41 (4)
HH25MMS 054607.3 − 001330 10.3 47 (5)
HH111 055146.3 + 024830 8.7 69 (6)
HH46 082543.9 − 510036 5.3 112 (7)
BHR71 120136.3 − 650853 −4.5 48 (7)
HH54B 125550.3 − 765623 2.4 (8)
IRAS16293 163222.8 − 242836 4.0 45 (1)
L483 181729.9 − 043939 5.4 49 (1)
S68N 182948.0 + 011646 8.8 45 (1)
SERSMM1 182949.8 + 011521 8.5 39 (1)
SERSMM4 182956.6 + 011315 8.1 33 (1)
B335 193700.9 + 073410 8.3 42 (1)
N7129FIR2 214301.7 + 660324 9.5 52 (9)
CEPE 230313.1 + 614226 −13.0 56 (10)

Notes.All central positions as in van Dishoeck et al. (2011) except S68N, which has an offset of 9′′. See Table 2 for the offsets of the observed positions;

(a)

bolometric temperature as defined by Myers & Ladd (1993) and estimated using data from Spitzer telescope observations (Velusamy et al. 2007; Evans et al. 2009; Gutermuth et al. 2009; Rebull et al. 2010), AKARI (Ishihara et al. 2010; Yamamura et al. 2010), IRAS (Beichman et al. 1988; Hurt & Barsony 1996), and JCMT (Di Francesco et al. 2008).

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