Large grains in discs around young stars: ATCA observations of WW Chamaeleontis, RU Lupi, and CS Chamaeleontis

Free Access

Table 1:

Source list of sources observed with the ATCA.
Source	Cloud	Distance^a	Age^b	Luminosity^b	Mass^b	Spectral	Position^d
		(pc)	(Myr)	( $L_\odot$ )	( $M_\odot$ )	type^c
WW Cha	Cha I	$160\pm15$	0.4-0.8	2.2	0.6-0.8	K5	(11:10:00.7, -76:34:59)
RU Lup	Lup II	$140\pm20$	0.04-0.5	2.1	2.0-2.8	K7-M0	(15:56:42.3, -37:49:15.47)
CS Cha	Cha I	$160\pm15$	2-3	1.3	0.9-1.2	K4	(11:02:25.1, -77:33:35.95)

^a Distances from Whittet et al. (1997) (WW Cha and CS Cha) and Hughes et al. (1993) (RU Lup); ^b ages, luminosities and masses from Hughes et al. (1994) (RU Lup) and Lawson et al. (1996) (WW Cha and CS Cha); ^c spectral types from Gauvin & Strom (1992) (WW Cha and CS Cha) and Hughes et al. (1994) (RU Lup); ^d RA and dec positions (J2000) from SIMBAD.

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.