Grain growth across protoplanetary discs: 10 μm silicate feature versus millimetre slope

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Volume 515 (June 2010)

A&A, 515 (2010) A77

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Table 2:

List of sources observed with the SMA, ATCA, CARMA, and VLA.
Source	RA	Dec	Sp. T.	Cloud	Spitzer	1 mm	3 mm	7 mm	Comments
	(J2000)	(J2000)
Vela
HBC 553	08 08 22.2	-36 03 47.0	M1.5	Vela	Wright	--	--	--
HBC 556	08 10 30.9	-36 01 46.5	M4	Vela	Wright	--	ATCA	ATCA
HBC 557	08 12 47.0	-36 19 18.0	K3:	Vela	Wright	--	ATCA	ATCA
HBC 559	08 13 56.1	-36 08 02.1		Vela	Wright	--	ATCA	ATCA
HBC 560	08 14 21.9	-36 10 03.4	K8	Vela	Wright	--	--	--
HBC 561	08 15 55.3	-35 57 58.1	K8	Vela	Wright	--	--	--	Binary^a
Chamaeleon
SZ Cha	10 58 16.9	-77 17 17.6	K0e	Cha I	GTO	--	ATCA
Sz 32	11 09 53.4	-76 34 25.5	K4.7	Cha I	c2d	--	ATCA	ATCA
Lupus
IK Lup	15 39 27.8	-34 46 17.2	K7	Lupus 1	Wright	SMA	ATCA	--	Binary^b
Sz 66	15 39 28.3	-34 46 18.0	M2	Lupus 1	Wright	SMA	ATCA	--	Binary^b
HM Lup	15 47 50.6	-35 28 35.3	M4	Lupus 1	c2d	SMA	--	--
Sz 73	15 47 56.9	-35 14 34.7	M0	Lupus 1	c2d	SMA	--	--
HN Lup	15 48 05.2	-35 15 52.8	M1.5	Lupus 1	Wright	SMA	--	--
Sz 76	15 49 30.7	-35 49 51.4	M1	Lupus 1	c2d	SMA	--	--
Sz 77	15 51 47.0	-35 56 42.8	M0	Lupus 1	Wright	SMA	--	--
IM Lup	15 56 09.2	-37 56 05.9	M0	Lupus 2	c2d	SMA^c	ATCA^c	ATCA
RY Lup	15 59 28.4	-40 21 51.2	G0V:	Lupus 3	c2d	SMA	ATCA	ATCA
MY Lup	16 00 44.6	-41 55 29.6		Lupus 4	Wright	SMA	ATCA	ATCA
EX Lup	16 03 05.5	-40 18 25.3	M0	Lupus 3	c2d	SMA	--	--
Sz 91	16 07 11.6	-39 03 47.1	M0.5	Lupus 3	--	SMA	--	--	Cold disc
Sz 96	16 08 12.6	-39 08 33.3	M1.5	Lupus 3	c2d	SMA	--	--
Sz 102	16 08 29.7	-39 03 11.0	K:e	Lupus 3	c2d	SMA	--	--
Sz 111	16 08 54.7	-39 37 43.1	M1.5	Lupus 3	--	SMA	ATCA	ATCA	Cold disc
SSTc2d J161029.57-392214.7	16 10 29.6	-39 22 14.7		Lupus 3	c2d	SMA	--	--	Cold disc
SSTc2d J161159.81-382338.5	16 11 59.8	-38 23 38.5		Lupus 3	c2d	SMA	--	--
RX J1615.3-3255	16 15 20.2	-32 55 05.0	K5	Isolated	c2d	SMA	ATCA	ATCA
Serpens
VV Ser	18 28 47.9	+00 08 40.0	A2e	Serpens	c2d	CARMA	CARMA	VLA	Herbig Ae
SSTc2d J182850.20+000949.7	18 28 50.2	+00 09 49.7	M5 $\pm$ 4	Serpens	c2d	CARMA	CARMA	VLA
SSTc2d J182858.08+001724.4	18 28 58.1	+00 17 24.4	G3 $\pm$ 5	Serpens	c2d	CARMA	CARMA	--	Cold disc
SSTc2d J182900.88+002931.5	18 29 00.9	+00 29 31.5	K7 $\pm$ 2	Serpens	c2d	CARMA	CARMA	VLA
CoKu Ser-G3	18 29 01.8	+00 29 54.6	K0 $\pm$ 7	Serpens	c2d	CARMA	CARMA	VLA
IRAS 18268-0025	18 29 28.1	-00 22 58		Serpens	c2d	CARMA	CARMA	VLA
SSTc2d J182936.19+004216.7	18 29 36.2	+00 42 16.7	F9 $\pm$ 5	Serpens	c2d	CARMA	CARMA	--
SSTc2d J182944.10+003356.1	18 29 44.1	+00 33 56.1	M0 $\pm$ 1.5	Serpens	Pontoppidan	CARMA	CARMA	--	Cold disc
EC 82	18 29 56.8	+01 14 46.0	M0	Serpens	c2d	CARMA	CARMA	VLA
EC 90	18 29 57.5	+01 14 07	M4 $\pm$ 2	Serpens	c2d	CARMA	CARMA	VLA	Binary^d
EC 97	18 29 58.2	+01 15 22		Serpens	c2d	CARMA	--	VLA
GSC 00446-00153	18 30 06.9	+00 42 34	F3V	Serpens	--	CARMA	CARMA	--
Corona Australis
S CrA	19 01 08.6	-36 57 20.0	K3	CrA	Wright	SMA	ATCA	ATCA	Binary^e
DG CrA	19 01 55.2	-37 23 40.5		CrA	Wright	SMA	ATCA	ATCA
VV CrA	19 03 06.7	-37 12 49.7	K7	CrA	Wright	SMA	ATCA	ATCA	Binary^f

Notes. ^(a) Separation $0\hbox{$.\!\!^{\prime\prime}$ }63$ (Correia et al. 2006); ^(b) IK Lup (Sz 65) and Sz 66 form a binary with a separation of $6\hbox{$.\!\!^{\prime\prime}$ }4$ (this work); ^(c) published in Lommen et al. (2007); ^(d) separation $1\hbox{$.\!\!^{\prime\prime}$ }5$ (e.g., Ciardi et al. 2005, and references therein); ^(e) separation $1\hbox{$.\!\!^{\prime\prime}$ }3$ (e.g., Forbrich et al. 2007, and references therein); ^(f) separation $2\hbox{$.\!\!^{\prime\prime}$ }0$ (this work).

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