Open Access

Table 8

Comparison of detected HCN masers and corresponding infrared photon luminosities.

Source (1) J (2) (v1, v2, v3) (3) SIR (Jy) (4) LIR (s−1) (5) Lm (s−1) (6) LIR/LM (7)
IR = 12 µm vs. 14 µm
IRC+10216 2−1 (0, 11e, 0) 4.75 × 104 1 .4 × 1046 2.6 × 1043 531
2−1 (0, 11f, 0) 4.75 × 104 1.9 × 1046 2.9 × 1042 6745
3−2 (0, 11e, 0) 4.75 × 104 1.8 × 1046 9.3 × 1042 1950
4−3 (0, 11f, 0) 4.75 × 104 2.4 × 1046 2.8 × 1043 874
RAFGL 4211 2−1 (0, 11e, 0) 7.93 × 102 1 .2 × 1046 1.4 × 1044 85
4−3 (0, 11e, 0) 7.93 × 102 2.0 × 1045 1.1 × 1043 181
II Lup 2−1 (0, 11e, 0) 1.32 × 103 8.5 × 1045 8.0 × 1043 107
4−3 (0, 11f, 0) 1.32 × 103 1 .2 × 1046 4.3 × 1043 282
R Vol 2−1 (0, 11e, 0) 2.03 × 102 2.0 × 1045 1.3 × 1043 151
2−1 (0, 11f, 0) 2.03 × 102 3.0 × 1045 2.9 × 1042 1052
3−2 (0, 11e, 0) 2.03 × 102 1 .2 × 1045 3.9 × 1042 303
4−3 (0, 11e, 0) 2.03 × 102 1 .1 × 1045 3.9 × 1042 293
AQ Sgr 3−2 (0, 11e, 0) 56.6 9.9 × 1043 2.0 × 1041 506
CRL 3068 2−1 (0, 11e, 0) 7.07 × 102 2.2 × 1046 2.0 × 1044 111
4−3 (0, 11f, 0) 7.07 × 102 2.1 × 1046 3.5 × 1044 60
V636 Mon 2−1 (0, 11e, 0) 1.25 × 102 5.8 × 1044 3.1 × 1042 188
IRC +20370 2−1 (0, 11e, 0) 5.34 × 102 5.6 × 1045 3.3 × 1043 172
3−2 (0, 11e, 0) 5.34 × 102 7.4 × 1045 2.5 × 1043 299
W Ori 2−1 (0, 11e, 0) 1.84 × 102 1 .0 × 1044 1.8 × 1042 56
3−2 (0, 11e, 0) 1.84× 102 1 .2 × 1044 2.0 × 1042 59
4−3 (0, 11e, 0) 1.84× 102 8.7 × 1043 5.1 × 1041 169
S Aur 2−1 (0, 11e, 0) 1.62 × 102 1 .9 × 1044 2.6 × 1042 73
V Aql 3−2 (0, 11e, 0) 1.50 × 102 2.0 × 1044 8.7 × 1041 228
RV Aqr 2−1 (0, 11e, 0) 3.08 × 102 1 .1 × 1045 1.0 × 1043 107
2−1 (0, 11f, 0) 3.08 × 102 9.7 × 1044 1.5 × 1042 638
3−2 (0, 11e, 0) 3.08 × 102 1 .0 × 1045 9.8 × 1042 133
IR = 4.6 µm vs. 5 µm
RAFGL 4211 3−2 (0, 31e, 0) 42.6 1.1 × 1045 3.8 × 1042 289
IR = 12 µm vs. 7 µm
RAFGL 4211 3−2 (0, 2, 0) 7.93 × 102 4.1 × 1045 7.8 × 1042 533

Notes. (1) Source name. (2) Rotational levels. (3) Vibrational states. (4) Flux density at corresponding infrared wavelength. (5) Photon rates at a wavelength range according to the velocity range given by maser line (see Table 6). (6) Photon rates in the corresponding maser line. (7) Ratios between the infrared photon and HCN maser luminosities.

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