The (w)hole survey: An unbiased sample study of transition disk candidates based on Spitzer catalogs

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Table 7

Comparison cavity radii with literature values.


ID	Name			Type^a	Ref.	ID	Name			Type^a	Ref.



1	TCha	140	19	I	1	51	IRS48	120	60	I	13
3	RECX5	10	33	M	2	52	DoAr44	80	30	I	10
4	CHXR22E	45	7	M	3	54	SR21	60	36	I	8
6	CSCha	60	38	M	4	60	oph62	2⁺²	3	M	6
9	T54	120	37	M	3	64	J160421	70	80	I	14
10	T21	190_-10	146	M	3	120	J182911	10	8	M	6
11	SZCha	30	29	M	3	127	Serp127	80	25	M	6
12	T35	15	15	M	3	128	J182935	25	7	M	6
14	T56	10	18	M	3	135	DMTau	4	18	I	10
15	CRCha	1⁺¹	10	M	4	136	UXTauA	50	25	I	10
18	T25	30	8	M	3	142	MWC758	25	73	I	10
21	HD142527	110	100	I	5	148	IPTau	100	2	M	4
24	Lup60	16	3	M	6	153	RYTau	2⁺²	26^b	I	15
27	Sz91	120	97	I	7	159	ABAur	1⁺⁴	115	I	16
29	Sz84	70	55	M	6	161	ASR118	2⁺⁴	1	M	6
33	HD135344	80	46	I	8	165	J034227	8	5	M	6
35	Sz76	2⁺²	1	M	9	168	J034434	5	3	M	6
38	RXJ1615	10	30	I	10	169	IC348LRL190	2⁺²	5	M	6
39	V4046Sgr	16	29	I	11	173	LkH-alpha330	120	68	I	10
45	SR24S	50	30	I	10	309	TWHya	10	4	M	17
46	RXJ1633	20	27	I	12	325	LkCa15	80	50	I	10
48	WSB60	8	15	I	10	326	CoKu-Tau-4	6	10	M	18
50	J162245	2⁺²	1	M	6	329	GMAur	30	20	I	10

Notes.

^(a)

M = derived from SED modeling, I = derived from millimeter imaging.

^(b)

This value is not a real cavity size, but a transition radius: the disk was fit with a surface density profile that radially increases and decreases, peaking at 26 AU.

Reference. (1) Huélamo et al. (2015); (2) Bouwman et al. (2010); (3) Kim et al. (2009); (4) Espaillat et al. (2011); (5) Fukagawa et al. (2013); (6) Merín et al. (2010); (7) Canovas et al. (2015); (8) Brown et al. (2009); (9) Padgett et al. (2006); (10) Andrews et al. (2011); (11) Rosenfeld et al. (2013); (12) Cieza et al. (2012a); (13) van der Marel et al. (2013); (14) Mathews et al. (2012); (15) Isella et al. (2010a); (16) Piétu et al. (2005); (17) Andrews et al. (2012); (18) D’Alessio et al. (2005).

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