b The maps of these sources are not complete or confused with other sources.
c These sources are detected with CO J=3-2 or higher.
d These outflows without corresponding young stellar objects.
e The underlined R is quoted from references.
f This source includes NGC7538 IRS1, IRS9, IRS11, and A.
g The distance is one of the assumed values 
g  (cf. Odenwald & Schwartz, 1993ApJ...405..706O).
h The mass is calculated under optical thick.
i This reference proposes that 05358+3543 consists of CO flow A, B 
i  and a SiO flow C.
j The authors of Ref. 326 proposed that this source has 2 overlapping outflows.
k The HH objects detected before 1999 were all from Reipurth (<V/104>)
l This source includes RNO43S and RNO43N.
m The parameters are derived from C^18^O observation.
n This source includes IC1396N BIMA1 and BIMA2.
o {dot}(M)_f_ is not used if it is deduced by M/{tau}.
p It was not identified as bipolar outflow by Ref. 191.
q Kelly & Macdonald (1996MNRAS.282..401K) reported that there may be two 
q  outflows.
r Its reshift lobe is probably masked by the outflow of L379 IRAS(3).
s This timescale is calculated with the assumption that the clump has a 
s  tangential velocity of 200km/s.
t This source includes NGC2024 Fir 4, 5 and 6.
u This source includes NGC7129 FIRS2-MM1, FIRS2-IR, FIRS1-IRS6 and FIRS1-MM1.
v Parameters calculated here are not for the whole outflow but only for 
v  the n4 region.
w The author of Ref. 354 (Mitchell, et al., 1995ApJ...438..794M) proposed that 
w  outflows at this position are not driven by FIR sources but by jets from 
w  faint undetected yet low-mass stars; the parameters in Table 1a are the total
w  of three outflows identified.