Properties of the molecular wind toward star-forming clump #1.2 S.
|(km s−1)||(1056 erg)||(1049 dyn s)||(1056 erg)||(1049 dyn s)||(1043 erg s−1)||(1035 dyn)|
|1.2 S (b)||199 ± 28||4.7||2.4||7.1||5.0||2.6||2.0|
Notes. The columns are: velocity offset between the wind and systemic component, Δv; energy (EΔv) and momentum (PΔv) derived from the observed velocity offsets; energy (Eσ) and momentum (Pσ) corresponding to the observed line widths; energy and momentum injection rates, dESF/dt and dPSF/dt, from star formation. Momentum and energy injection rates are normalized to an outflow timescale of 50 Myr. We provide a measurement uncertainty only for the velocity offset. For the other estimates, typical measurement uncertainties are between 10 and 20%, and likely much smaller than the astrophysical uncertainties, which are difficult to quantify accurately.
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.