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Home All issues Volume 600 (April 2017) A&A, 600 (2017) A99 Full HTML
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Table A.7

Mass-accretion rate, the luminosity of [O i] in the 63  μm line, and mass-loss rate calculated from it.

Name Ṁacc L[O i 63 μm] Ṁw Name Ṁacc L[O i 63 μm] Ṁ w
(M⊙ yr-1) (L⊙) (M⊙ yr-1) (M⊙ yr-1) (L⊙) (M⊙ yr-1)
AQU 01 1.7 × 10-06 8.3 × 10-04 8.3 × 10-08 AQU 02 5.9 × 10-06 8.2 × 10-04 8.2 × 10-08
AQU 03 − a − b − AQU 04 8.4 × 10-07 − b −
AQU 05 1.6 × 10-06 − b − AQU 06 8.1 × 10-07 − b −
CHA 01 − a 3.7 × 10-04 3.7 × 10-08 CHA 02 2.3 × 10-07 8.7 × 10-05 8.7 × 10-09
CRA 01 1.6 × 10-06 1.2 × 10-03 1.2 × 10-07 OPH 01 − a 2.9 × 10-03c −
OPH 02 1.1 × 10-06 5.2 × 10-04 5.2 × 10-08 PER 01 2.9 × 10-06 3.4 × 10-03 3.4 × 10-07
PER 02 6.0 × 10-06 7.8 × 10-03 7.8 × 10-07 PER 04 7.6 × 10-07 5.3 × 10-04 5.3 × 10-08
PER 05 1.4 × 10-06 2.8 × 10-04 2.8 × 10-08 PER 06 9.2 × 10-07 1.6 × 10-03 1.6 × 10-07
PER 07 4.6 × 10-07 1.2 × 10-03 1.2 × 10-07 PER 08 2.2 × 10-06 1.1 × 10-02 1.1 × 10-06
PER 09 2.9 × 10-06 − e − PER 10 3.9 × 10-06 − e −
PER 12 6.9 × 10-07 1.1 × 10-04 1.1 × 10-08 PER 13 4.4 × 10-07 − b −
PER 14 2.4 × 10-07 4.6 × 10-04 4.6 × 10-08 PER 15 1.1 × 10-06 2.1 × 10-04 2.1 × 10-08
PER 16 7.4 × 10-07 2.6 × 10-04 2.6 × 10-08 PER 17 2.3 × 10-08 1.4 × 10-04 1.4 × 10-08
PER 18 3.4 × 10-07 1.8 × 10-03 1.8 × 10-07 PER 19 1.4 × 10-07 1.8 × 10-03 1.8 × 10-07
PER 20 1.4 × 10-06 1.9 × 10-03 1.9 × 10-07 PER 21 1.2 × 10-06 8.6 × 10-04 8.6 × 10-08
PER 22 1.6 × 10-06 1.0 × 10-03 1.0 × 10-07 SCO 01 − a 2.8 × 10-04 2.8 × 10-08
SERS 01 1.1 × 10-05 2.8 × 10-03 2.8 × 10-07 SERS 02 4.7 × 10-05 − e −
TAU 01 2.0 × 10-07 7.6 × 10-04 7.6 × 10-08 TAU 02 6.1 × 10-08 1.1 × 10-04 1.1 × 10-08
TAU 03 − a 5.4 × 10-05 5.4 × 10-09 TAU 04 1.8 × 10-07 4.5 × 10-04 4.5 × 10-08
TAU 06 7.3 × 10-08 9.6 × 10-05 9.6 × 10-09 TAU 07 − a 3.5 × 10-04 3.5 × 10-08
TAU 08 − a − f − TAU 09 − a 2.9 × 10-04 2.9 × 10-08
W40 01 − a 3.1 × 10-04c − W40 02 2.1 × 10-05 5.4 × 10-02 5.4 × 10-06
W40 03 − a 1.5 × 10-01c − W40 04 − a 1.1 × 10-01c −
W40 05 − a 7.8 × 10-02c − W40 06 − a − c,d −
W40 07 2.3 × 10-06 5.4 × 10-04 5.4 × 10-08 L1448-MM 5.8 × 10-06 2.2 × 10-03 2.2 × 10-07
IRAS03245+3002 4.2 × 10-06 6.4 × 10-04 6.4 × 10-08 L1455-IRS3 4.7 × 10-08 5.0 × 10-04 5.0 × 10-08
NGC 1333-IRAS2A 2.3 × 10-05 − b − NGC 1333-IRAS3A 5.4 × 10-06 − f −
NGC 1333-IRAS4A 5.9 × 10-06 1.5 × 10-03g − NGC 1333-IRAS4B 2.9 × 10-06 1.3 × 10-04 1.3 × 10-08
IRAS03301+3111 5.3 × 10-07 3.6 × 10-04 3.6 × 10-08 B1 a 3.5 × 10-07 1.9 × 10-04 1.9 × 10-08
B1 c 3.3 × 10-06 − b − L1489 4.9 × 10-07 2.2 × 10-04 2.2 × 10-08
L1551-IRS5 2.9 × 10-06 9.7 × 10-03 9.7 × 10-07 TMR1 4.9 × 10-07 1.1 × 10-03 1.1 × 10-07
TMC1A 3.5 × 10-07 3.3 × 10-03 3.3 × 10-07 L1527 1.2 × 10-06 1.8 × 10-03 1.8 × 10-07
TMC1 1.2 × 10-07 1.5 × 10-03 1.5 × 10-07 IRAM04191 7.1 × 10-08 2.4 × 10-04 2.4 × 10-08
HH46 3.6 × 10-06 5.1 × 10-03 5.1 × 10-07 Ced110-IRS4 5.2 × 10-07 1.3 × 10-03 1.3 × 10-07
BHR71 9.6 × 10-06 3.4 × 10-03 3.4 × 10-07 IRAS12496 4.6 × 10-06 5.9 × 10-03 5.9 × 10-07
IRAS15398 1.0 × 10-06 3.0 × 10-03 3.0 × 10-07 GSS30 1.8 × 10-06 5.1 × 10-03 5.1 × 10-07
VLA1623-243 1.7 × 10-06 1.3 × 10-03 1.3 × 10-07 WL12 2.1 × 10-07 7.9 × 10-04 7.9 × 10-08
Elias29 1.8 × 10-06 4.0 × 10-03 4.0 × 10-07 IRS44 6.6 × 10-07 4.8 × 10-04 4.8 × 10-08
IRS46 6.5 × 10-08 1.5 × 10-04 1.5 × 10-08 IRS63 1.3 × 10-07 3.3 × 10-04 3.3 × 10-08
RNO91 3.4 × 10-07 1.3 × 10-03 1.3 × 10-07 L483 6.6 × 10-06 1.1 × 10-03 1.1 × 10-07
Ser-SMM1 7.1 × 10-05 4.0 × 10-03 4.0 × 10-07 Ser-SMM4 4.4 × 10-06 1.8 × 10-02 1.8 × 10-06
Ser-SMM3 1.2 × 10-05 1.1 × 10-02 1.1 × 10-06 RCrA-IRS5A 9.2 × 10-07 1.2 × 10-03 1.2 × 10-07
RCrA I7A 1.2 × 10-05 8.9 × 10-03 8.9 × 10-07 RCrA I7B 6.0 × 10-06 2.4 × 10-03 2.4 × 10-07
HH100 2.3 × 10-06 − f − L723 2.3 × 10-06 1.3 × 10-04 1.3 × 10-08
B335 2.1 × 10-06 2.5 × 10-04 2.5 × 10-08 L1157 3.0 × 10-06 3.3 × 10-04 3.3 × 10-08

Notes.

(a)

Not Class 0/I.

(b)

Non-detection.

(c)

Dominated by PDR.

(d)

Line in absorption.

(e)

Dominated by neighbouring source.

(f)

Source not observed with PACS.

(g)

Only one off position was used due to possible contamination but this flux may still be underestimated.

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