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Table A.1

Observed C3H2c/l ratios toward various objects, and the associated physical conditions (visual extinction AV, medium density n, (rotational) temperature T) when available in the literature.

Source AV [ mag ] n [ cm-3 ] T rot a [ K ] c/l ratio Reference

Prestellar cores
TMC-1(CPb) 3 × 104 7 70 Cernicharo et al. (1991)
TMC-1(CP) 3 × 104 7 25 Turner et al. (2000)
TMC-1(CP) 3 × 104 7 2040 Kawaguchi et al. (1991)
TMC-1(CP) 3 × 104 7 28 Fossé et al. (2001)
TMC-1(edgec) 3 × 104 7 10 Fossé et al. (2001)
L183 50 Turner et al. (2000)
TMC-1C 7 (c), 4 (l) 67 Spezzano et al. (2016)
L1544 6 (c), 4 (l) 32 Spezzano et al. (2016)
Protostellar cores
L1527 7 × 105 12 12 Sakai & Yamamoto (2013)
Translucent clouds
CB17, CB24, CB228 17(average) Turner et al. (2000)
Circumstellar envelopes
IRC+10216 25 30 Cernicharo et al. (1991)
Diffuse clouds
W49N T CMB d 4 Kulczak-Jastrzȩbska et al. (2012)
W51 T CMB 13 Kulczak-Jastrzȩbska et al. (2012)
B0355+508, B0415+379, T CMB 1540 Liszt et al. (2012)
B2200+420, B2251+158
PDRs
Horsehead Nebula (edgee) < 104 f 35 Teyssier et al. (2005)
Horsehead Nebula (dense cloude) 10-20 2 × 105 f 15 Teyssier et al. (2005)
Orion Bar 17 (c), 26 (l) 34 Cuadrado et al. (2015)

Notes.

(a)

The rotational temperature of c and/or lC3H2, which may not be equal to the kinetic temperature.

(b)

CP stands for cyanopolyyne peak.

(c)

The edge position is (−40, 0) offset from the CP position α2000 = 4h 41m 42.5s, δ2000 = 25° 41′ 27′′ (Kawaguchi et al. 1991).

(d)

TCMB stands for the temperature of the cosmic microwave background (2.7 K).

(e)

The edge and cloud positions are (by estimation) (−20, −15) and (−72, −62) offset from the (0, 0) position (Teyssier et al. 2005).

(f)

Density corresponds to the model presented by Pety et al. (2012).

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