Probing the role of protostellar feedback in clustered star formation - Mapping outflows in the collapsing protocluster NGC 2264-C

Home

All issues

Volume 499 / No 1 (May III 2009)

A&A, 499 1 (2009) 175-189

Full HTML

Highlight

Free Access

Table 5:

Global properties of the population of eleven ¹²CO(2-1) outflows observed in NGC 2264-C.
$M_{\rm {tot}}$	$P_{\rm {tot}}$	$F_{\rm {tot}}$	$E_{\rm {tot}}$	$L_{\rm {tot}}$
(10^-2 $M_\odot$ )	( $M_\odot$ km s^-1)	(10^-5 $M_\odot$ km s^-1 yr^-1)	(10⁴⁴ erg)	( $L{_{\odot}}$ )
⁽¹⁾	⁽²⁾	⁽³⁾	⁽⁴⁾	⁽⁵⁾
3 - 189	3.8-11	30-170	3.4-10	0.2-1.2

⁽¹⁾ Minimum and maximum total mass of outflow-entrained gas, computed from the individual outflow masses given in Table 4.
⁽²⁾ Minimum and maximum total outflow momentum, computed from the individual outflow momenta given in Table 4 ( $P_{\rm {tot}}$ = $\sum \limits_{\rm flows}$ $P_{\rm {flow}}$ ).
⁽³⁾ Minimum and maximum total outflow momentum flux ( $F_{\rm {tot}}$ = $\sum \limits_{\rm flows}$ $F_{\rm {flow}}$ ).
⁽⁴⁾ Minimum and maximum total kinetic energy of the outflows.
⁽⁵⁾ Minimum and maximum total mechanical luminosity of the outflow population.

Source LaTeX | All tables | In the text

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.