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Table 2

Isotopic ratios resulting from our LTE analysis with CASSIS and directly from line ratios.

Isotopologues Column-density 3σ ratio Line ratio
ratio range and 3σ error

12C/13C = 3.8 ± 1.0 [89.3]

HC3N, H13CCCN, HC13CCN+HCC13CN 4.3 3.3–5.6 4.1±1.1
CCH, 13CCH, C13CH 3.0 2.2–3.4
CN, 13CNa 2.3 2.1–2.6
CS, 13CS 4.6 3.1–7.0 3.4±0.2
HCO+, H13CO+ 2.5 1.8–4.2 2.1±0.1
HCN, H13CN 2.0 1.6–2.6 1.7–2.7b
CO, 13CO 4.0 3.0–5.3
CH3OH, 13CH3OHc 3.8 2.9–4.9 3.8±0.6
CH3CN, 13CH3CNa,c 1.5 1.2–2.8 4.3±0.1
H2CO, HCOd 6.5 4.4–9.7 4.0±0.2
HNC, HN13C 6.2 4.3–8.5 2.1±0.1
C18O, 13C18O 5.0 2.5–16.6

13C/14C > 141

H13CN, H14CN >142
13CO, 14CO >72

14N/15N = 20 ± 10 [441]e

CN, C15Nb 44.8 24.0–190.0
N2H+, 15NNH+, N15NH+ 14.6 >5.3 16.2±9.5
HCN, HC15N 12.8 10.1–17.0 11.1±0.3
HNC, H15NC 30.8 15.2–67.0 15.9±1.7
NS, 15NS >17.4
HC3N, HCN >7.6
13CN, 13C15N >37.0
H13CN, H13C15N 18.4 13.8–27.5 16.3±1.4
HN13C, H15N13C 13.9±6.2
HC3N, HCN >7.6
13CN×3.8f, C15N 69.1 49.0–106.0
H13CN×3.8f, HC15N 23.6 19.0–30.8 24.4±1.1
HN13C×3.8f, 15HNC 55.1 30.4–84.4 26.2±2.3

16O/18O = 36 ± 14 [498.8]

CO, C18O 36.7 26.2–60.0 24.5±2.7
SiO, Si18O 12.1 9.3–16.7 11.5±2.3
HCO+, HC18O+ 53.1 >25.0 15.3±8.1
SO, S18O >16.5
H2CO, H2C18Od >71.6
13CO, 13C18O 69.2 >32.0 40.2±19.7
13CO×3.8f, C18O 52.1 35.3–76.0 37.4±6.2
H13CO+ × 3.8f, HC18O+ 86.5 39.9–534.7 35.4±18.8

18O/17O 5 [5.4]

Si18O, Si17O >7.7 2.8±2.3
C18O, C17O 5.5 4.9–8.3 4.7±4.1

28Si, 29Si, 30Si:28Si/29Si = 6.7 ± 0.4 [19.7];29Si/30Si  = 1.0 ± 0.1 [0.7]

SiO, 29SiO 7.3 5.7–9.4 6.6±0.5
SiS, 29SiS 7.7 >2.3
SiO, 30SiO 8.9 6.7–11.8 6.7±0.7
29SiO, 30SiO 1.2 1.0–1.5 1.0±0.1

32S, 33S, 34S:32S/34S = 14 ± 3 [22.5];32S/33S > 34 [126.6]

CS, C33S >34.0
CS, C34S 23.5 14.4–41.5 13.9±3.3
SO, 34SO 14.1 >5.5
NS, N34S 35.3 >15.0
13CS×3.8f, C34S 19.0 11.8–37.2 14.1±7.2

Notes. The headlines with isotopic ratios in boldface indicate the most likely values of the ratios in CK Vul, as discussed in the text. The values given in square brackets correspond to solar system isotopic ratios from Lodders (2003).

(a)

Very poor fit.

(b)

We obtain different ratios for different transition pairs and therefore the values were not averaged.

(c)

Analysis performed at the fixed A to E ratio of 1.

(d)

Only ortho transitions were analyzed.

(e)

Marty et al. (2011) measured a 14N/15N ratio of 441 for the solar wind. The value of 272.3 in Lodders (2003) corresponds to terrestrial ratio.

(f)

As explained in the text, the ratios were transformed with the average 12C/13C ratio.

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