Volatile-carbon locking and release in protoplanetary disks - A study of TW Hya and HD 100546

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Volume 592 (August 2016)

A&A, 592 (2016) A83

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Table C.1

Line fluxes in units of 10^-18W m^-2.

Line	HD 100546	Ref.	TW Hya	Ref.

CO 2–1	(–)		0.082 ± 0.016	^g
CO 3–2	1.72 ± 0.01	^a	0.43 ± 0.13	^g
CO 6–5	16.1 ± 0.8	^a ^b	2.5 ± 0.8	^a ^b
CO 7–6	23.5 ± 2.7	^c	(–)
CO 8–7	33.1 ± 3.5	^c	(–)
CO 9–8	45.3 ± 4.1	^c	(–)
CO 10–9	55.3 ± 3.7	^c	3.4 ± 0.6	^h
CO 11–10	51.3 ± 4.5	^c	(–)
CO 12–11	58.3 ± 3.3	^c	(–)
CO 13–12	60.7 ± 4.7	^c	(–)
CO 14–13	60.0 ± 8.3	^d	(–)
CO 15–14	88.3 ± 9.7	^d	(–)
CO 16–15	58.8 ± 9.7	^d	(–)
CO 17–16	73.9 ± 10.0	^d	(–)
CO 18–17	71.5 ± 6.9	^d	3.5 ± 1.2	ⁱ
CO 19–18	64.7 ± 8.5	^d	(–)
CO 20–19	49.9 ± 5.7	^d	(–)
CO 21–20	65.0 ± 8.8	^d	(–)
CO 22–21	≤ 42.0	^d	(–)
CO 23–22	78.4 ± 11.0	^d	≤ 4.4	^j
CO 24–23	71.3 ± 12.0	^d	(–)
CO 25–24	≤ 77.1	^d	(–)
CO 28–27	81.5 ± 11.0	^d	(–)
CO 29–28	78.6 ± 19.0	^d	≤ 3.4	ⁱ
CO 30–29	73.4 ± 15.0	^d	(–)
CO 31–30	≤ 140.0	^d	(–)
CO 32–31	≤ 65.3	^d	(–)
CO 33–32	≤ 84.5	^d	≤ 8.3	ⁱ
CO 34–33	53.1 ± 14.0	^d	(–)
CO 35–34	≤ 44.1	^d	(–)
CO 36–35	52.9 ± 13.0	^d	≤ 4.2	ⁱ
CO 37–36	≤ 82.9	^d	(–)
CO 38–37	≤ 107.0	^d	(–)
¹³CO 2–1	(–)		0.020 ± 0.001	^k
¹³CO 3–2	≤ 0.66	^e	0.044 ± 0.013	^l
¹³CO 6–5	≤ 7.5	^c	(–)
¹³CO 7–6	≤ 7.2	^c	(–)
¹³CO 8–7	≤ 10.2	^c	(–)
¹³CO 9–8	≤ 14.4	^c	(–)
¹³CO 10–9	(–)		0.28 ± 0.04	^h
¹³CO 11–10	16.8 ± 3.4	^c	(–)
¹³CO 12–11	(–)		(–)
C¹⁸O 2–1	(–)		0.006 ± 0.001	^k
HD 112 μm	≤ 27.0	^a	6.3 ± 0.7	^j
HD 56 μm	≤ 160.0	^a	3.1 ± 1.0	ⁿ
CI 1–0	0.66 ± 0.07	^a^b	0.067 ± 0.018	^a^b
CI 2–1	≤ 3.58	^a	≤ 0.9	^a
CII 158 μm	135.0 ± 15.0	^d^f	≤ 6.6	^m
OI 145 μm	357.0 ± 13.0	^d^f	≤ 5.5	^m
OI 63 μm	5540.0 ± 50.0	^d^e	36.5 ± 12.1	^m
C₂H	≤ 0.005	^a	0.017 ± 0.008	^a
C₂H	≤ 0.005	^a	0.020 ± 0.008	^a
C₂H	≤ 0.005	^a	0.019 ± 0.008	^a
C₂H	≤ 0.005	^a	0.024 ± 0.008	^a

Notes.

^(a)

This work;

^(b)

Kama et al. (2016);

^(c)

van der Wiel et al. (2014);

^(d)

Meeus et al. (2013);

^(e)

Panić et al. (2010);

^(f)

Fedele et al. (2013b);

^(g)

Qi et al. (2004);

^(h)

Fedele (2016);

⁽ⁱ⁾

Kamp et al. (2013);

^(j)

Bergin et al. (2013);

^(k)

Favre et al. (2013);

^(l)

Thi et al. (2004);

^(m)

Thi et al. (2010);

⁽ⁿ⁾

Fedele (in prep.).

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