Table 1
Molecular outflow properties.
| Sources | R out | V out | M out | Ṁ out |
|
L out |
|
|
Ṗ out |
|
|
| (pc) | (km s-1) | ( M⊙) | ( M⊙ yr-1) | – | ( L⊙) | – | – | (g cm s-2) | – | – | |
|
|
|||||||||||
| NGC 1614 | 560 | 360 | 3.2 × 107 | 40 | 0.8 | 6.5 × 108 | 0.06 | >0.05a | 1.4 × 1035 | 1.9 | >65a |
|
|
|||||||||||
| IRAS 17208 | 160 | 600 | 4.6 × 107 | 330 | 1.4 b | 1.6 × 1010 | 0.4 b | >6c | 1.6 × 1036 | 5 | > 5 × 103 c |
| – | – | – | – | 2.0 d | – | 0.6 d | 0.02 e | – | – | 17 e | |
Notes. All properties are derived for the line wing components as defined in Sects. 4.1 and 4.4 assuming α = 33° and 35° in Eqs. (1), (3), and (4) for NGC 1614 and IRAS 17208-0014, respectively. Outflow mass rates, momentum rates, and kinetic luminosities have uncertainties of ±0.34 dex, ±0.36 dex, and ±0.40 dex, respectively. The mass, momentum, and energy loading factors have associated uncertainties of ±0.43 dex. See Sect. 5.3 for details.
Derived assuming 
(González-Martín et al. 2009).
Derived assuming 
(Aalto et al. 2015b.).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.