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Table A.1.
Cooling curves implemented in MPI-AMRVAC with basic properties and references.
Name | Tmin | Tmax | T at Λmax | Λmax | Λ (106 K) | τr (106 K) | τnl (106 K) | Reference and notes |
---|---|---|---|---|---|---|---|---|
Unit | K | K | K | erg cm3 s−1 | erg cm3 s−1 | s | ||
cloudy_ism | 101 | 109 | 105 | 10−21.28 | 10−21.87 | 2963 | 0.026 | Ferland et al. (1998), ISM metallicity |
cloudy_solar | 101 | 109 | 105 | 10−21.25 | 10−21.79 | 2431 | 0.029 | Ferland et al. (1998), solar metallicity |
Colgan | 104.06 | 109.06 | 105.29 | 10−21.09 | 10−21.31 | 803 | 0.117 | Colgan et al. (2008) |
Colgan_DM | 101 | 109.06 | 105.29 | 10−21.09 | 10−21.31 | 803 | 0.117 | Colgan et al. (2008) |
Dere_corona | 104 | 109 | 105.35 | 10−21.18 | 10−21.4 | 1008 | 0.135 | Dere et al. (2009), coronal abundances |
Dere_corona_DM | 101 | 109 | 105.35 | 10−21.18 | 10−21.4 | 1008 | 0.135 | Dere et al. (2009), coronal abundances |
Dere_photo | 104 | 109 | 105.35 | 10−21.25 | 10−21.93 | 3364 | 0.047 | Dere et al. (2009), photospheric abundances |
Dere_photo_DM | 101 | 109 | 105.35 | 10−21.25 | 10−21.93 | 3364 | 0.047 | Dere et al. (2009), photospheric abundances |
DM | 102 | 109 | 105.3 | 10−21.06 | 10−22.28 | 7411 | 0.012 | Dalgarno & McCray (1972) |
FM | 103 | 1010 | 105.6 | 10−21.06 | 10−21.26 | 720 | 0.253 | Hildner (1974), modified by Forbes & Malherbe (1991) |
Hildner | 103 | 108 | 104.9 | 10−21.1 | 10−22.28 | 7204 | 0.005 | Hildner (1974) |
JCcorona | 104 | 107.95 | 105.29 | 10−21.09 | 10−21.31 | 803 | 0.117 | Colgan et al. (2008), modified by Xia et al. (2011) |
Klimchuk | 103 | 108 | 104.97 | 10−21.02 | 10−21.72 | 2089 | 0.019 | Klimchuk et al. (2008) |
MB | 104 | 109 | 105.3 | 10−21.42 | 10−22.0 | 3969 | 0.052 | MacDonald & Bailey (1981) |
MLcosmol | 102 | 109 | 104.2 | 10−22.19 | 10−23.51 | 127268 | 0.001 | Mellema & Lundqvist (2002), zero metallicity |
MLsolar1 | 102 | 109 | 105.4 | 10−21.17 | 10−22.2 | 6192 | 0.024 | Mellema & Lundqvist (2002), solar metallicity |
MLwc | 102 | 109 | 105 | 10−18.46 | 10−20.23 | 68 | 0.002 | Mellema & Lundqvist (2002), WC-star metallicity |
Rosner | 103 | 108 | 105.4 | 10−21.2 | 10−21.94 | 3457 | 0.046 | Rosner et al. (1978), extended by Priest (1982) |
SPEX | 103.8 | 108.16 | 105.32 | 10−20.67 | 10−21.71 | 2023 | 0.019 | Schure et al. (2009) |
SPEX_DM | 101 | 108.16 | 105.32 | 10−20.67 | 10−21.71 | 2023 | 0.019 | Schure et al. (2009) |
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