Toward understanding the formation of multiple systems - A pilot IRAM-PdBI survey of Class 0 objects

Home

All issues

Volume 512 (March-April 2010)

A&A, 512 (2010) A40

Full HTML

Highlight

Free Access

Table 3:

Properties of the 1.3 mm continuum sources detected in the high-resolution PdBI maps.
Source	Position (1.3 mm)		Peak flux	FWHM¹	Flux density²	Separation³
	$\alpha$ (J2000)	$\delta$ (J2000)	(mJy/beam)	(arcsec)	(mJy)	(AU)
L1448-C	03:25:38.87	30:44:05.3	59 $\pm$ 0.9	0.9 $\pm$ 0.05	57 $\pm$ 2	-
L1448-C / South1	03:25:38.95	30:44:03.2	11 $\pm$ 0.7	0.7 $\pm$ 0.1	11 $\pm$ 2	600
NGC 1333-IRS2A	03:28:55.56	31:14:37.1	26 $\pm$ 1.16	0.55 $\pm$ 0.07	18 $\pm$ 2	-
NGC 1333-IRS2A / SE	03:28:56.00	31:14:33.1	7 $\pm$ 1.16	0.23 $\pm$ 0.04	4 $\pm$ 1.5	1900
IRAM 04191	04:21:56.90	15:29:46.1	2 $\pm$ 0.37	0.28 $\pm$ 0.02	0.9 $\pm$ 0.4	-
L1527	04:39:53.87	26:03:09.8	50 $\pm$ 1.2	0.42 $\pm$ 0.05	65 $\pm$ 3	-
L1521-F	04:28:38.94	26:51:35.2	1 $\pm$ 0.12	0.65 $\pm$ 0.009	0.8 $\pm$ 0.2	-

Notes. ⁽¹⁾ FWHM diameter is computed from a circular Gaussian fit to the visibilities.
⁽²⁾ Flux integrated above the 3 $\sigma$ level.
⁽³⁾ Projected distance to the primary source.

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.