GIARPS High-resolution Observations of T Tauri stars (GHOsT) - IV. Accretion properties of the Taurus-Auriga young association

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Volume 667 (November 2022)

A&A, 667 (2022) A124

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Table 1

Disk properties of the selected accreting CTTs for this study, based on ALMA observations.

Source	i_disk^(a) [deg]	M_disk,dust [M_⊕]	R_eff,68% [au]	Disk type^(b)	Source	i_disk^(a) [deg]	M_disk,dust [M_⊕]	R_eff,68% [au]	Disk type^(b)
BP Tau	38.2⁽¹⁾	7.8⁽¹⁾	29⁽¹⁾	Full⁽¹⁾	GI Tau	43.8⁽¹⁾	3.1 ⁽¹⁾	18⁽¹⁾	Full⁽¹⁾
CI Tau	50⁽¹⁾	37.0⁽¹⁾		Sub⁽¹⁾	GK Tau	40.2⁽¹⁾	0.89⁽¹⁾	8⁽¹⁾	Full⁽¹⁾
CQ Tau	29⁽³⁾	41.0⁽³⁾	63⁽³⁾	TD⁽³⁾	GM Aur	53⁽³⁾	43⁽³⁾	76⁽³⁾	TD⁽³⁾
CW Tau	59⁽⁴⁾	11⁽⁴⁾	46⁽⁴⁾	Full⁽⁴⁾	HN Tau	69.8⁽¹⁾	2.7⁽¹⁾	15⁽¹⁾	Full⁽¹⁾
CY Tau	–	14⁽⁵⁾	48⁽⁵⁾	Full^(c)	HQ Tau	53.8⁽¹⁾	1.1⁽¹⁾	20⁽¹⁾	Full⁽¹⁾
DE Tau	–	5.2⁽⁷⁾	22⁽⁷⁾	Full^(c)	IP Tau	45.2⁽¹⁾	2.6⁽¹⁾	30⁽¹⁾	TD⁽¹⁾
DF Tau	52⁽⁶⁾	0.65⁽⁶⁾	–	Full^(c)	IQ Tau	62.1 ⁽¹⁾		55⁽¹⁾	Sub⁽¹⁾
DG Tau	37⁽⁴⁾	–	–	Full⁽⁴⁾	LkCa 15	–	33⁽³⁾	124⁽³⁾	TD⁽³⁾
DH Tau	16.9⁽¹⁾	5.1 ⁽¹⁾	14⁽¹⁾	TD⁽⁹⁾	MWC480	36.5⁽¹⁾	73⁽¹⁾	55⁽¹⁾	Sub⁽¹⁾
DK Tau	12.8⁽¹⁾	5.2⁽¹⁾		Full⁽¹⁾	RW Aur A	55.1 ⁽¹⁾	7.2⁽¹⁾	14⁽¹⁾	Full⁽¹⁾
DL Tau	45.0⁽¹⁾	45⁽¹⁾		Sub⁽¹⁾	RY Tau	65⁽¹⁾	39⁽¹⁾	50⁽¹⁾	TD⁽¹⁾
DN Tau	35.2⁽¹⁾	15⁽¹⁾	39⁽¹⁾	Sub⁽¹⁾	SU Aur	–	7.1⁽⁸⁾	50⁽⁸⁾	Full^(c)
DO Tau	27.6⁽¹⁾	25⁽¹⁾	25⁽¹⁾	Full⁽¹⁾	UX Tau	39⁽⁵⁾	–	–	TD⁽⁹⁾
DQ Tau	16.1⁽¹⁾	28⁽¹⁾	24⁽¹⁾	Full⁽¹⁾	UY Aur	23.5⁽¹⁾	5⁽¹⁾	5⁽¹⁾	Sub⁽¹⁰⁾
DR Tau	5.4⁽¹⁾	50⁽¹⁾	36⁽¹⁾	Full⁽¹⁾	UZ Tau E	56.1 ⁽¹⁾	24⁽¹⁾	59⁽¹⁾	Sub⁽¹⁾
DS Tau	65.2⁽¹⁾	5.8⁽¹⁾	59⁽¹⁾	Sub⁽¹⁾	V409 Tau	69.3⁽¹⁾	3.6⁽¹⁾	31 ⁽¹⁾	Full⁽¹⁾
FT Tau	35.5⁽¹⁾	15⁽¹⁾	33⁽¹⁾	Sub⁽¹⁾	V807 Tau	–	1.6⁽⁸⁾	12⁽⁸⁾	TD⁽⁹⁾
GG Tau A	57⁽³⁾	–	–	Full^(c)	V836 Tau	43.1 ⁽¹⁾	7.8⁽¹⁾	21 ⁽¹⁾	Full⁽¹⁾
GH Tau	–	0.69–0.51⁽⁸⁾	12⁽⁸⁾	Full⁽⁹⁾

Notes. ^(a)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. ^(b)Full: disk without substructures, Sub: disk with substructures (e.g. inner hole, gaps and rings), TD: transitional disk. ^(c)Classification adopted from Esplin & Luhman (2019), based on the mid-IR SED.

References. ⁽¹⁾Long et al. (2019),⁽²⁾Antonellini et al. (2020), ⁽³⁾Francis & van der Marel (2020), ⁽⁴⁾Bacciotti et al. (2018), ⁽⁵⁾Tripathi et al. (2017),⁽⁶⁾ Andrews et al. (2013), ⁽⁷⁾Simon et al. (2019), ⁽⁸⁾Akeson et al. (2019), ⁽⁹⁾Currie & Sicilia-Aguilar (2011),⁽¹⁰⁾Tang et al. (2014).

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