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cloudy-agn/reference/old_cloudy_linelist/caution_0410.txt
othocaeS 3bd8f6e0b9 merged emission line lists.
2016-05-12 17:08:03 -04:00

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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 *
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