Science/cloudy-agn
1
0
Fork 0
mirror of https://asciireactor.com/otho/cloudy-agn.git synced 2025-01-18 23:45:05 +00:00
Code Issues Packages Projects Releases Wiki Activity
73103fe5cf
cloudy-agn/reference/linelist/caution_0410.txt
caes c1359aca9d Added References and Line Lists
2015-10-13 02:26:13 -04:00

215 lines
18 KiB
Plaintext
Raw Blame History

This file contains invisible Unicode characters

This file contains invisible Unicode characters that are indistinguishable to humans but may be processed differently by a computer. If you think that this is intentional, you can safely ignore this warning. Use the Escape button to reveal them.

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 *
Reference in New Issue View Git Blame Copy Permalink