GIARPS High-resolution Observations of T Tauri stars (GHOsT) - I. Jet line emission

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Table 1

Source properties.

Source	d	SpT	A_V	L_*	L_acc	M_*	log (M_acc)	i_disk
	(pc)		(mag)	(L_⊙)	(L_⊙)	(M_⊙)	(M_⊙ yr⁻¹)	(deg)
RY Tau	128 ± 4⁽¹⁾	F7⁽¹⁾	1.8⁽²⁾	10.7⁽²⁾	–	2.04⁽³⁾	−7.3⁽⁴⁾	65⁽¹⁾

DG Tau	121 ± 18⁽⁵⁾	K7.0⁽²⁾	1.60⁽²⁾	0.5⁽²⁾	0.09⁽⁶⁾	0.76⁽⁶⁾	−8.12⁽⁶⁾	37⁽⁷⁾

DL Tau	159 ± 8⁽⁵⁾	K5.5⁽²⁾	1.80⁽²⁾	0.5⁽²⁾	0.14⁽⁶⁾	0.75⁽⁸⁾	−8.06⁽⁶⁾	45⁽¹⁾

HN Tau	145 ± 19⁽⁵⁾	K3⁽²⁾	1.15⁽²⁾	0.16⁽²⁾	0.05⁽⁶⁾	0.78⁽⁸⁾	−8.69⁽⁶⁾	70⁽³⁾

DO Tau	139 ± 7⁽⁵⁾	M0.3⁽²⁾	0.75⁽²⁾	0.22⁽²⁾	0.1⁽⁶⁾	0.56⁽⁸⁾	−8.21⁽⁶⁾	28⁽³⁾

RW Aur A	163 ± 10⁽⁵⁾	K0⁽²⁾	0−2^(2,9)	0.72⁽²⁾	–	1.48⁽⁸⁾	−7.39⁽¹⁰⁾	55⁽³⁾

References. ⁽¹⁾ Long et al. (2018); ⁽²⁾ Herczeg & Hillenbrand (2014): ⁽³⁾ Long et al. (2019); ⁽⁴⁾ Skinner et al. (2018); ⁽⁵⁾ Gaia Collaboration (2018); ⁽⁶⁾ Simon et al. (2016); ⁽⁷⁾ Bacciotti et al. (2018); ⁽⁸⁾ Rigliaco et al. 2015 and references therein; ⁽⁹⁾Koutoulaki et al. (2019); ⁽¹⁰⁾Facchini et al. (2016).

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