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 2:

Observed properties of the ¹²CO(2-1) outflows detected in the map of Fig. 2.
OUTFLOW	Local systemic ⁽¹⁾	Outflow main ⁽²⁾		Area ⁽³⁾	Length ⁽⁴⁾
LOBE	velocity ${V_{\rm sys}}$	LSR velocities interval
	(km s^-1)	(km s^-1)		(arcsec²)	(arcsec)
		V₁	V₂
F1 (Red)	7.5	28.5	13	2780	127
F2 (Blue)	7.6	-27	1.1	3060	184
F3 (Blue)	7.4	-26.6	1.4	1935	70
F4 (Red)	7.7	23	14.3	900	53
F5 (Blue)	7.3	-12	0.3	1080	50
F6 (Red)	7.1	28.1	13.1	1360	56
F7 (Red)	7.2	33.2	14.7	2230	72
F8 (Blue)	7.2	-23	1.7	590	38
F9 (Red)	7.2	30.2	13.7	800	53
F10 (Red)	7.2	32.2	13.7	610	50
F11 (Red)	7.7	33	15.2	4180	90

⁽¹⁾ Systemic LSR velocity of the ambient material around each outflow.
⁽²⁾ Velocity interval [V₁; V₂] over which each outflow emission is detected but no significant emission is seen in the reference spectrum.
⁽³⁾ Surface area of each outflow lobe.
⁽⁴⁾ Major size of each outflow lobe.

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.