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

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Volume 533 (September 2011)

A&A, 533 (2011) A112

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Table E.2

Equivalent widths and fluxes in selected lines^a.

Star	Comp^b	P(2) 4682.64		P(5) 4708.77		P(8) 4735.87		P(11) 4763.99		P(17) 4823.3109		P(26) 4920.41		¹³CO R(15) 4650.4256
		EW	flux	EW	flux	EW	flux	EW	flux	EW	flux	EW	flux	EW	flux

L1551 IRS5	N	9.9 (1.3)	0.61	15.3 (1.3)	0.95	18.6 (0.6)	1.16	17.5 (1.8)	1.1	–	–	–	–	2.7 (0.3)	0.16
Elias 29	N	3.2 (0.1)	1.2	1.95 (0.13)	0.74	3.1 (0.1)	1.2	2.6 (0.2)	0.99	2.9 (0.3)	1.2	–	–	0.32 (0.7)	0.12
RNO 91¹	B	15 (3)	0.23	10 (4)	0.16	18 (3)	0.28	–	–	18 (2)	0.29	–	–
HH 100 IRS	B	6.8 (0.4)	1.2	4.8 (0.3)	0.86	6.6 (0.3)	1.2	5.6 (0.4)	1.01	–	–	7.2 (0.5)	1.3	–	–
HH 100 IRS	N	23 (2)	4.1	42.6 (3)	7.6	53 (3)	9.5	57 (3)	10.2	40 (3)	7.4	–	–	0.29 (0.3)	0.051
GSS 30	Blue	19.1 (0.1)	6.9	25.2 (0.1)	9.1	27.5 (0.1)	10.0	27. 6(0.3)	10.1	–	–	–	–	3.3 (0.2)	1.16
GSS 30	Red	24.0 (0.3)	8.6	27.0 (0.3)	9.7	37.5 (0.3)	13.6	45.8 (0.4)	16.7	–	–	12.1 (0.4)²	²4.7	<2³	<0.7³
IRS 44 W	Blue	36.5 (2.0)	0.42	–	–	–	–	–	–	33 (2)	0.52	–	–	5.4 (1.3)	0.082
IRS 44 W	Red	91 (8)	2.6	67 (7)	1.9	67 (8)	1.9	47 (9)	1.3	80 (10)	2.3	–	–	–	–
CrA IRS 2	T	14.4 (0.7)	1.2	18.2 (0.3)	1.5	21.1 (0.4)	1.8	24.2 (0.4)	2.1	23.9 (0.2)⁴	2.1⁴	18.6 (0.2)	1.6	1.6 (0.2)	0.25
IRS 43 S	T	17.6 (2)	0.44	5.9 (2)	0.15	8.7 (1)	0.22	11 (2)	0.27	19 (2)	0.50	–	–	–	–
HL Tau	T	7.2 (1.0)	0.63	9.7 (1.0)	0.84	11.0 (1.0)	0.95	13.9 (0.7)	1.2	18.2 (0.6)	1.6	–	–	–	–
IRS 63	B	16 (2)	0.31	–	–	8 (3)	0.16	10 (3)	0.20	–	–	14 (3)	0.30
IRS 63	N	10 (2)	0.20	4.7 (1.5)	0.10	11.6 (2)	0.24	–	–	–	–	–	–
SVS 20 S	N	5.5 (3)	0.30	4.3 (1.3)	0.24	6.7 (1.0)	0.37	3.8 (1.6)	0.21	–	–	2.3 (0.7)	0.13	–	–
TMC 1A	B	21 (5)	0.32	–	–	16 (3)	0.26	–	–	–	–	–	–

WL 12		Low S/N
SVS 20 N		Low S/N
TMC 1A	N	Low S/N
WL 6		No CO emission detected
Elias 32		No CO emission detected
IRS 44 E		No CO emission detected
IRS 43 N		No CO emission detected

Notes.

⁽¹⁾

Equivalent width (~2-σ error) in km s^-1 and Flux in 10^-14 erg cm-2 s^-1 for 6 ¹²CO and 1 ¹³CO line.

^(a)

Fluxes are calculated from line equivalent widths and continuum flux, and are overestimated when continuum is spatially extended beyond the slit width. Flux uncertainty also includes ~30% relative uncertainty in continuum flux across the M-band.

^(b)

Component, Br = broad, N = Narrow, NB = Narrow Blue, T = Total.

⁽²⁾

P(37) 5.053 μm.

⁽³⁾

Upper limit from other ¹³CO lines because R(15) from GSS 30 has a high upper limit.

⁽⁴⁾

P(18) 4.834 μm.

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