GIARPS High-resolution Observations of T Tauri stars (GHOsT) - II. Connecting atomic and molecular winds in protoplanetary disks

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Volume 643 (November 2020)

A&A, 643 (2020) A32

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This article has 2 errata:
[https://doi.org/10.1051/tpe/2021006]
[https://doi.org/10.1051/0004-6361/202038534e]

Table 2

Source properties.

Source	RA	Dec	d ^(a)	SpT	A_v	L_⋆	M_⋆	i_disk ^(b)
	[J2000]	[J2000]	[pc]		[mag]	[L_⊙]	[M_⊙]	[deg]
BP Tau	04:19:15.83	+29:06:26.93	129	M0.5 ⁽¹⁾	0.45 ⁽¹⁾	0.42 ⁽¹⁾	0.52 ⁽²⁾	38.2 ⁽²⁾
CI Tau	04:33:52.01	+22:50:30.09	158	K5.5 ⁽¹⁾	1.90 ⁽¹⁾	0.63 ⁽¹⁾	0.90 ⁽³⁾	50.0 ⁽⁴⁾
CoKu HP Tau G2	04:35:54.15	+22:54:13.40	166	G2 ⁽¹⁾	2.55 ⁽¹⁾	6.92 ⁽¹⁾	...	50 ⁽⁵⁾
CQ Tau	05:35:58.47	+24:44:54.09	163	F5 ⁽⁶⁾	1.89 ⁽⁷⁾	11.94 ⁽⁷⁾	1.75 ⁽⁷⁾	29 ⁽⁸⁾
CW Tau	04:14:17.00	+28:10:57.76	132	K3.0 ⁽¹⁾	1.80 ⁽¹⁾	0.45 ⁽¹⁾	1.01 ⁽³⁾	59 ⁽⁹⁾
DD Tau	04:18:31.13	+28:16:29.16	123	M4.8 ⁽¹⁾	0.75 ⁽¹⁾	0.29 ⁽¹⁾	0.13 ⁽¹⁾	...
DF Tau	04:27:02.79	+25:42:22.46	124	M2.7 ⁽¹⁾	0.10 ⁽¹⁾	0.91 ⁽¹⁾	0.32 ⁽³⁾	52 ⁽³⁾
DG Tau	04:27:04.69	+26:06:16.04	121	K7.0 ⁽¹⁾	1.60 ⁽¹⁾	0.51 ⁽¹⁾	0.76 ⁽³⁾	37 ⁽⁹⁾
DH Tau	04:29:41.56	+26:32:58.27	135	M2.3 ⁽¹⁾	0.65 ⁽¹⁾	0.22 ⁽¹⁾	0.41 ⁽³⁾	16.9 ⁽²⁾
DK Tau	04:30:44.25	+26:01:24.47	128	K8.5 ⁽¹⁾	0.70 ⁽¹⁾	0.54 ⁽¹⁾	0.68 ⁽³⁾	12.8 ⁽²⁾
DL Tau	04:33:39.08	+25:20:38.10	159	K5.5 ⁽¹⁾	1.80 ⁽¹⁾	0.50 ⁽¹⁾	0.98 ⁽²⁾	45.0 ⁽²⁾
DN Tau	04:35:27.38	+24:14:58.91	128	M0.3 ⁽¹⁾	0.55 ⁽¹⁾	0.83 ⁽¹⁾	0.55 ⁽³⁾	35.2 ⁽⁴⁾
DO Tau	04:38:28.59	+26:10:49.47	139	M0.3 ⁽¹⁾	0.75 ⁽¹⁾	0.22 ⁽¹⁾	0.59 ⁽²⁾	27.6 ⁽²⁾
DQ Tau	04:46:53.06	+17:00:00.13	197	M0.6 ⁽¹⁾	1.40 ⁽¹⁾	1.17 ⁽²⁾	1.61 ⁽²⁾	16.1 ⁽²⁾
DR Tau	04:47:06.21	+16:58:42.81	196	K6c ⁽¹⁾	0.45 ⁽¹⁾	0.32 ⁽¹⁾	0.93 ⁽²⁾	5.4 ⁽²⁾
DS Tau	04:47:48.59	+29:25:11.19	159	M0.4 ⁽¹⁾	0.25 ⁽¹⁾	0.19 ⁽¹⁾	0.69 ⁽³⁾	65.2 ⁽⁴⁾
FT Tau	04:23:39.19	+24:56:14.11	128	M2.8 ⁽¹⁾	1.30 ⁽¹⁾	0.18 ⁽¹⁾	0.34 ⁽²⁾	35.5 ⁽²⁾
GG Tau	04:32:30.33	+17:31:40.83	140	K7.5 ⁽¹⁾	1.00 ⁽¹⁾	1.41 ⁽¹⁾	0.62 ⁽¹⁾	57 ⁽¹⁰⁾
GH Tau	04:33:06.22	+24:09:33.63	130 ⁽¹¹⁾	M2.3 ⁽¹⁾	0.40 ⁽¹⁾	0.64 ⁽¹⁾	0.36 ⁽¹²⁾	...
GI Tau	04:33:34.06	+24:21:17.07	130	M0.4 ⁽¹⁾	2.05 ⁽¹⁾	0.56 ⁽¹⁾	0.52 ⁽²⁾	43.8 ⁽²⁾
GK Tau	04:33:34.56	+24:21:05.85	129	K6.5 ⁽¹⁾	1.50 ⁽¹⁾	0.93 ⁽¹⁾	0.69 ⁽³⁾	40.2 ⁽²⁾
GM Aur	04:55:10.98	+30:21:59.37	159	K6 ⁽³⁾	0.30 ⁽¹⁾	0.49 ⁽¹⁾	0.88 ⁽³⁾	53.21 ⁽¹³⁾
HL Tau	04:31:38.44	+18:13:57.65	140	K3c ⁽¹⁾	2.50 ⁽¹⁾	0.14 ⁽¹⁾	1.8 ⁽¹⁴⁾	47 ⁽¹⁴⁾
HN Tau	04:33:39.36	+17:51:52.30	145	K3 ⁽¹⁾	1.15 ⁽¹⁾	0.17 ⁽¹⁾	1.53 ⁽²⁾	69.8 ⁽²⁾
HQ Tau	04:35:47.33	+22:50:21.64	158	K2.0 ⁽¹⁾	2.60 ⁽¹⁾	4.47 ⁽¹⁾	1.53 ⁽³⁾	53.8 ⁽²⁾
IP Tau	04:24:57.08	+27:11:56.54	130	M0.6 ⁽¹⁾	0.75 ⁽¹⁾	0.39 ⁽¹⁾	0.59 ⁽³⁾	45.2 ⁽⁴⁾
IQ Tau	04:29:51.56	+26:06:44.85	131	M1.1 ⁽¹⁾	0.85 ⁽¹⁾	0.24 ⁽¹⁾	0.50 ⁽²⁾	62.1 ⁽²⁾
MWC480	04:58:46.26	+29:50:36.99	161	A4.5 ⁽⁴⁾	0.10 ⁽²⁾	17.38 ⁽¹⁾	1.91 ⁽²⁾	36.5 ⁽²⁾
RW Aur A	05:07:49.54	+30:24:05.07	163	K0 ⁽¹⁾	0-2 ^(1,15)	0.72 ⁽¹⁾	1.20 ⁽²⁾	55.1 ⁽²⁾
RY Tau	04:21:57.41	+28:26:35.53	128	F7 ⁽⁴⁾	1.85 ⁽¹⁾	10.71 ⁽¹⁾	2.04 ⁽²⁾	65.0 ⁽²⁾
UX Tau	04:30:04.00	+18:13:49.43	139 ⁽¹¹⁾	M1.9 ⁽¹⁾	0.40 ⁽¹⁾	0.37 ⁽¹⁾	1.51 ⁽³⁾	39.0 ⁽¹²⁾
UY Aur	04:51:47.39	+30:47:13.55	155	K7.0 ⁽¹⁾	1.00 ⁽¹⁾	0.85 ⁽¹⁾	0.65 ⁽²⁾	23.5 ⁽²⁾
UZ Tau E	04:32:43.02	+25:52:30.90	131	M1.9 ⁽¹⁾	0.90 ⁽¹⁾	0.40 ⁽¹⁾	1.23 ⁽²⁾	56.1 ⁽²⁾
V409 Tau	04:18:10.78	+25:19:57.38	131	M0.6 ⁽¹⁾	1.00 ⁽¹⁾	0.66 ⁽¹⁾	0.50 ⁽²⁾	69.3 ⁽²⁾
V836 Tau	05:03:06.60	+25:23:19.60	169	M0.8 ⁽¹⁾	0.60 ⁽¹⁾	0.30 ⁽¹⁾	0.58 ⁽³⁾	43.1 ⁽²⁾
XZ Tau	04:31:40.09	+18:13:56.64	144 ⁽¹¹⁾	M2 ⁽¹⁶⁾	1.40 ⁽¹⁶⁾	0.42 ⁽¹⁶⁾	0.36 ⁽¹⁶⁾	35 ⁽¹⁷⁾

Notes. ^(a) The distance for each target is computed from the Gaia DR2 parallax (Gaia Collaboration 2018). ^(b) Disk inclinations are measured from ALMA observations and refer to the outer disk. An exception is made for GG Tau, where the inclination of the resolved inner disk is reported.

References. ⁽¹⁾ Herczeg & Hillenbrand (2014), ⁽²⁾ Long et al. (2019), ⁽³⁾ Simon et al. (2016), ⁽⁴⁾ Long et al. (2018), ⁽⁵⁾ Bouvier et al. (1995), ⁽⁶⁾ Varga et al. (2018), ⁽⁷⁾ Villebrun et al. (2019), ⁽⁸⁾ Chapillon et al. (2008), ⁽⁹⁾ Bacciotti et al. (2018), ¹⁰ Francis & van der Marel (2020), ⁽¹¹⁾Akeson et al. (2019), ⁽¹²⁾Banzatti et al. (2019), ⁽¹³⁾Huang et al. (2020), ⁽¹⁴⁾Yen et al. (2019), ⁽¹⁵⁾Koutoulaki et al. (2019), ⁽¹⁶⁾Hartigan & Kenyon (2003), ⁽¹⁷⁾Osorio et al. (2016).

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