Disks and outflows in CO rovibrational emission from embedded, low-mass young stellar objects

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Table 8

Inner radius of disk CO emission^a.

Target	FWHM ^a	v _inner ^b	R_in(sini)²^c	Incl.^d
	km s^-1	km s^-1	(AU)	°

Broad Emission
IRS 63	92	70	0.17	33
HH 100 IRS	80	61	0.23	28
IRS 43 S	146	111	0.070	58
CrA IRS 2	54	41	0.49	19
WL 12	98	74	0.16	34
HL Tau	130	99	0.088	49
TMC 1A	96	73	0.16	34
SVS 20 N	100	76	0.15	35
RNO 91	165	125	0.056	71

Narrow Emission^e
GSS 30	42	32	0.87	–
HH 100 IRS	11	8.4	13	–
Elias 29	18	13	5.3	–
IRS 63	28	21	2.0	–
CrA IRS 2	34	26	1.3	–
IRS 44 W	32	24	1.5	–
IRS 43 S	42	32	0.87	–
L1551 IRS 5	12	11	7.3	–

Notes.

^(a)

CO v = 2−1 emission;

^(b)

half-width at 20% the peak of a Gaussian with listed FWHM;

^(c)

assumes M_∗ = M_⊙;

^(d)

inclination if the inner radius of CO emission is 0.050 AU;

^(e)

narrow component may not be in Keplerian rotation.

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