710044: C-This is the last iteration and H 1 Ly(a) optical depth changed by 84% (was 1.19e+07). Try another iteration. 710045- !Charge transfer ionization of H reached 99.4% of the local H ionization rate. 710046- !Photoionization of upper level of Mg II 2798 reached 100.0% of the total Mg+ photo rate. 710047- !Photoionization of upper levels of [O I] reached 15.1% of the total O destruction rate. 710048- !Photoionization of upper levels of [O III] reached 12.8% of the total O++ photo rate. 710049- !The largest plasma frequency was 2.46e-07 Ryd = 3.70e+05 micron The continuum is set to 0 below this. 710050- !The largest continuum brightness temperature was 5.165e+03K at 9.109e-03 Ryd. 710051- !AGE: Cloud age was not set. Longest timescale was 2.00e+03 s. 710052- !The excitation temp of Lya exceeded the electron temp, largest value was 1.81e+04K (gas temp there was 1.38e+04K, zone 141) 710053- !Some iso-structure lines mased: He-like HELI, line 12-11 had optical depth -1.60e+00 710054- !Some iso-structure lines mased: He-like HELI, line 20-17 had optical depth -8.03e-01 710055- !Some iso-structure lines mased: He-like HELI, line 29-27 had optical depth -1.29e+00 710056- !Some iso-structure lines mased: He-like HELI, line 30-25 had optical depth -7.92e-01 710057- !Some iso-structure lines mased: He-like HELI, line 39-37 had optical depth -4.13e-01 710058- !Some iso-structure lines mased: He-like HELI, line 41-39 had optical depth -2.04e-01 710059- !Some iso-structure lines mased: He-like HELI, line 42-35 had optical depth -4.19e-01 710060- !Some iso-structure lines mased: He-like HELI, line 51-49 had optical depth -1.32e-01 710061- !Some iso-structure lines mased: He-like HELI, line 56-47 had optical depth -2.21e-01 710062- !Some iso-structure lines mased: He-like HELI, line 72-61 had optical depth -1.27e-01 710063- !The CMB was not included. This is added with the CMB command. 710064- !The ratio of radiation to gas pressure reached 7.95e-01 at zone 135. Caused by Lyman alpha. 710065- !The radiation pressure jumped by 224% at zone 140, from 8.67e-02 to 2.47e-02 to 2.37e-02 710066- Charge transfer heating reached 2.98% of the local heating. 710067- The largest continuum occupation number was 7.075e+02 at 2.341e-07 Ryd. 710068- Photoionization of Ca+ 2D level by Ly-alpha reached 87.3% of the total rate out. 710069- G-bar cooling lines reached 1.18% of the local cooling. Line=Mn 2 2589A 710070- Line absorption heating reached 1.65% of the local heating. 710071- Bound Compton heating reached 2.80% of the local heating. 710072- Rate of induced H 2-photon emission reached 1.02e-01 s^-1 710073- Induced recombination was 85.5% of the total for H level170 710074- Stimulated emission was 99.5% of the total for H transition171 -170 710075- Timescale-photoerosion of Fe=4.94e+06 yr 710076- The Balmer continuum optical depth was 1.26e-01. 710077- The Balmer continuum stimulated emission correction to optical depths reached 1.41e-01. 710078- The continuum optical depth at the lowest energy considered (1.055e-08 Ryd) was 4.569e+10. 710079- The optical depth to electron scattering is 0.074 710080- 710081- *********************************> Cloudy 08.00 <********************************** 710082- * table agn * 710083- * phi(h) 19.750000 range 0.999466 7354000.000000 * 710084- * grid from 19.0 to 19.75 in 0.25 dex steps * 710085- * HDEN=9.750000 * -- 919519: C-This is the last iteration and H 1 Ly(a) optical depth changed by 98% (was 5.72e+06). Try another iteration. 919520- !Photoionization of upper level of Mg II 2798 reached 10.6% of the total Mg+ photo rate. 919521- !Photoionization of upper levels of [O III] reached 12.4% of the total O++ photo rate. 919522- !The largest plasma frequency was 7.78e-07 Ryd = 1.17e+05 micron The continuum is set to 0 below this. 919523- !The largest continuum brightness temperature was 2.904e+04K at 9.109e-03 Ryd. 919524- !AGE: Cloud age was not set. Longest timescale was 1.61e+02 s. 919525- !The excitation temp of Lya exceeded the electron temp, largest value was 2.38e+04K (gas temp there was 1.32e+04K, zone 154) 919526- !Some iso-structure lines mased: He-like HELI, line 20-17 had optical depth -3.44e-01 919527- !Some iso-structure lines mased: He-like HELI, line 30-25 had optical depth -8.74e-01 919528- !Some iso-structure lines mased: He-like HELI, line 42-35 had optical depth -5.27e-01 919529- !Some iso-structure lines mased: He-like HELI, line 56-47 had optical depth -3.03e-01 919530- !Some iso-structure lines mased: He-like HELI, line 72-61 had optical depth -1.57e-01 919531- !The CMB was not included. This is added with the CMB command. 919532- !The ratio of radiation to gas pressure reached 6.42e-01 at zone 157. Caused by Lyman alpha. 919533- !The radiation pressure jumped by 290% at zone 162, from 3.20e-01 to 6.58e-02 to 6.17e-02 919534- Continuum fluorescent production of H-beta was significant. 919535- Photoionization of upper levels of [O I] reached 4.3% of the total O destruction rate. 919536- The largest continuum occupation number was 2.295e+03 at 7.032e-07 Ryd. 919537- The continuum brightness temperature fell below 10,000K at 6.985e+00 microns. 919538- Photoionization of Ca+ 2D level by Ly-alpha reached 70.3% of the total rate out. 919539- Line absorption heating reached 1.99% of the local heating. 919540- Rate of induced H 2-photon emission reached 5.45e-01 s^-1 919541- Induced recombination was 97.1% of the total for H level170 919542- Stimulated emission was 99.9% of the total for H transition171 -170 919543- Timescale-photoerosion of Fe=8.78e+05 yr 919544- Induced recombination cooling was 1.5% of the total. 919545- Free-free heating was 6.1% of the total. 919546- The Balmer continuum optical depth was 3.39e-01. 919547- The Balmer continuum stimulated emission correction to optical depths reached 1.52e-01. 919548- The continuum optical depth at the lowest energy considered (1.055e-08 Ryd) was 5.897e+11. 919549- The optical depth to electron scattering is 0.073 919550- Line radiation pressure capped by thermalization length. 919551- 919552- *********************************> Cloudy 08.00 <********************************** 919553- * table agn * 919554- * phi(h) 20.500000 range 0.999466 7354000.000000 * 919555- * grid from 20.0 to 20.75 in 0.25 dex steps * 919556- * HDEN=10.750000 * 919557- * grid from 7.0 to 14.0 in 0.25 dex steps * 919558- * normalize to "inci" 1215 scale factor = 1215 * 919559- * C * 919560- * atom H-like element hydrogen levels resolved 18 * -- 981567: C-This is the last iteration and C 6 Bal(a) optical depth changed by 20.6% (was 1.32e+00). Try another iteration. 981568- !Photoionization of upper levels of [O III] reached 12.9% of the total O++ photo rate. 981569- !The largest plasma frequency was 7.78e-07 Ryd = 1.17e+05 micron The continuum is set to 0 below this. 981570- !The largest continuum brightness temperature was 5.165e+04K at 9.109e-03 Ryd. 981571- !AGE: Cloud age was not set. Longest timescale was 1.49e+02 s. 981572- !The excitation temp of Lya exceeded the electron temp, largest value was 2.36e+04K (gas temp there was 1.49e+04K, zone 162) 981573- !Some iso-structure lines mased: He-like HELI, line 12-11 had optical depth -7.88e-01 981574- !Some iso-structure lines mased: He-like HELI, line 19-17 had optical depth -1.92e-01 981575- !Some iso-structure lines mased: He-like HELI, line 20-17 had optical depth -4.74e-01 981576- !Some iso-structure lines mased: He-like HELI, line 29-27 had optical depth -2.18e-01 981577- !Some iso-structure lines mased: He-like HELI, line 30-25 had optical depth -6.46e-01 981578- !Some iso-structure lines mased: He-like HELI, line 42-35 had optical depth -3.18e-01 981579- !Some iso-structure lines mased: He-like HELI, line 56-47 had optical depth -1.76e-01 981580- !The CMB was not included. This is added with the CMB command. 981581- !The ratio of radiation to gas pressure reached 6.48e-01 at zone 165. Caused by Lyman alpha. 981582- !The radiation pressure jumped by 174% at zone 3, from 6.81e-06 to 2.95e-05 to 9.61e-05 981583- Continuum fluorescent production of H-beta was significant. 981584- Photoionization of upper level of Mg II 2798 reached 2.5% of the total Mg+ photo rate. 981585- Photoionization of upper levels of [O I] reached 2.7% of the total O destruction rate. 981586- The largest continuum occupation number was 4.081e+03 at 7.032e-07 Ryd. 981587- The continuum brightness temperature fell below 10,000K at 5.777e+00 microns. 981588- Photoionization of Ca+ 2D level by Ly-alpha reached 76.5% of the total rate out. 981589- Line absorption heating reached 2.37% of the local heating. 981590- Rate of induced H 2-photon emission reached 9.68e-01 s^-1 981591- Induced recombination was 98.3% of the total for H level170 981592- Stimulated emission was 99.9% of the total for H transition171 -170 981593- Timescale-photoerosion of Fe=4.94e+05 yr 981594- Induced recombination cooling was 1.4% of the total. 981595- Free-free heating was 6.3% of the total. 981596- The Balmer continuum optical depth was 1.36e-01. 981597- The Balmer continuum stimulated emission correction to optical depths reached 1.48e-01. 981598- The continuum optical depth at the lowest energy considered (1.055e-08 Ryd) was 4.269e+11. 981599- The optical depth to electron scattering is 0.074 981600- Line radiation pressure capped by thermalization length. 981601- 981602- *********************************> Cloudy 08.00 <********************************** 981603- * table agn * 981604- * phi(h) 20.750000 range 0.999466 7354000.000000 * 981605- * grid from 20.0 to 20.75 in 0.25 dex steps * 981606- * HDEN=10.750000 * 981607- * grid from 7.0 to 14.0 in 0.25 dex steps * 981608- * normalize to "inci" 1215 scale factor = 1215 * -- 1329800: C-This is the last iteration and He 2 Ly(a) optical depth changed by 28% (was 6.94e+04). Try another iteration. 1329801- !Continuum fluorescent production of H-beta was very important. 1329802- !Photoionization of upper levels of [O III] reached 14.6% of the total O++ photo rate. 1329803- !The largest plasma frequency was 1.85e-06 Ryd = 4.94e+04 micron The continuum is set to 0 below this. 1329804- !The largest continuum brightness temperature was 1.633e+06K at 9.109e-03 Ryd. 1329805- !AGE: Cloud age was not set. Longest timescale was 3.59e+01 s. 1329806- !The excitation temp of Lya exceeded the electron temp, largest value was 2.42e+04K (gas temp there was 2.22e+04K, zone 232) 1329807- !Rate of induced H 2-photon emission reached 3.05e+01 s^-1 1329808- !Free-free heating was 33.3% of the total. 1329809- !The CMB was not included. This is added with the CMB command. 1329810- !The ratio of radiation to gas pressure reached 8.20e-01 at zone 163. Caused by Lyman alpha. 1329811- !The radiation pressure jumped by 249% at zone 3, from 1.63e-05 to 1.05e-04 to 5.05e-04 1329812- Te-ne bounds of Case B lookup table exceeded, H I Case B line intensities set to zero. 1329813- The largest continuum occupation number was 8.228e+04 at 1.730e-06 Ryd. 1329814- The continuum occupation number fell below 1 at 1.714e+00 microns. 1329815- The continuum brightness temperature fell below 10,000K at 1.820e+00 microns. 1329816- Photoionization of Ca+ 2D level by Ly-alpha reached 43.8% of the total rate out. 1329817- Line absorption heating reached 2.15% of the global heating. 1329818- G-bar cooling lines reached 7.37% of the local cooling. Line=P 5 1121A 1329819- Line absorption heating reached 6.53% of the local heating. 1329820- Induced recombination was 99.9% of the total for H level170 1329821- Stimulated emission was 100.0% of the total for H transition171 -170 1329822- Timescale-photoerosion of Fe=1.56e+04 yr 1329823- Compton heating was 1.2% of the total. 1329824- Induced recombination cooling was 6.3% of the total. 1329825- The continuum optical depth at the lowest energy considered (1.055e-08 Ryd) was 1.168e+12. 1329826- The optical depth to electron scattering is 0.080 1329827- Line radiation pressure capped by thermalization length. 1329828- 1329829- *********************************> Cloudy 08.00 <********************************** 1329830- * table agn * 1329831- * phi(h) 22.250000 range 0.999466 7354000.000000 * 1329832- * grid from 22.0 to 22.75 in 0.25 dex steps * 1329833- * HDEN=11.500000 * 1329834- * grid from 7.0 to 14.0 in 0.25 dex steps * 1329835- * normalize to "inci" 1215 scale factor = 1215 * 1329836- * C * 1329837- * atom H-like element hydrogen levels resolved 18 * 1329838- * atom He-like element helium levels resolved 15 * 1329839- * atom H-like element helium levels resolved 15 * 1329840- * set nend 5000 * 1329841- * stop column density 23 * -- 1494646: C-This is the last iteration and He 2 Ly(a) optical depth changed by 32% (was 8.28e+04). Try another iteration. 1494647- !Continuum fluorescent production of H-beta was very important. 1494648- !Photoionization of upper levels of [O III] reached 16.5% of the total O++ photo rate. 1494649- !The largest plasma frequency was 5.84e-06 Ryd = 1.56e+04 micron The continuum is set to 0 below this. 1494650- !The largest continuum brightness temperature was 9.184e+06K at 9.109e-03 Ryd. 1494651- !AGE: Cloud age was not set. Longest timescale was 4.36e+00 s. 1494652- !G-bar cooling lines reached 23.72% of the local cooling. Line=O 3 698A 1494653- !Rate of induced H 2-photon emission reached 1.72e+02 s^-1 1494654- !Free-free heating was 64.8% of the total. 1494655- !The CMB was not included. This is added with the CMB command. 1494656- !The ratio of radiation to gas pressure reached 5.71e-01 at zone 176. Caused by Lyman alpha. 1494657- !The radiation pressure jumped by 334% at zone 3, from 0.00e+00 to 4.65e-05 to 3.10e-04 1494658- Thermal collisional ionization of H reached 1.80% of the local ionization rate. 1494659- Te-ne bounds of Case B lookup table exceeded, H I Case B line intensities set to zero. 1494660- Photoionization of upper levels of [O I] reached 1.3% of the total O destruction rate. 1494661- The largest continuum occupation number was 2.669e+05 at 5.196e-06 Ryd. 1494662- The continuum occupation number fell below 1 at 1.115e+00 microns. 1494663- The continuum brightness temperature fell below 10,000K at 1.024e+00 microns. 1494664- Photoionization of Ca+ 2D level by Ly-alpha reached 14.4% of the total rate out. 1494665- Line absorption heating reached 3.26% of the global heating. 1494666- Line absorption heating reached 7.52% of the local heating. 1494667- Induced recombination was 100.0% of the total for H level170 1494668- Stimulated emission was 100.0% of the total for H transition171 -170 1494669- Timescale-photoerosion of Fe=2.78e+03 yr 1494670- Induced recombination cooling was 14.9% of the total. 1494671- The Balmer continuum optical depth was 5.26e-02. 1494672- The continuum optical depth at the lowest energy considered (1.055e-08 Ryd) was 8.345e+12. 1494673- The continuum of the computed structure may be optically thick in the near infrared. 1494674- The optical depth to electron scattering is 0.080 1494675- Line radiation pressure capped by thermalization length. 1494676- 1494677- *********************************> Cloudy 08.00 <********************************** 1494678- * table agn * 1494679- * phi(h) 23.000000 range 0.999466 7354000.000000 * 1494680- * grid from 23.0 to 23.25 in 0.25 dex steps * 1494681- * HDEN=12.500000 * 1494682- * grid from 7.0 to 14.0 in 0.25 dex steps * 1494683- * normalize to "inci" 1215 scale factor = 1215 * 1494684- * C * 1494685- * atom H-like element hydrogen levels resolved 18 * 1494686- * atom He-like element helium levels resolved 15 * 1494687- * atom H-like element helium levels resolved 15 *