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Messages 579 - 608 of 889   Oldest  |  < Older  |  Newer >  |  Newest
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579
Hello, I've been constructing an xspec mtable/atable and have run into the problem below. Any ideas? Thanks, Alex. ... PROBLEM DISASTER An assert has been...
alexblustin
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Sep 1, 2008
10:45 am
580
Hi Alex, This problem has been solved. Please upgrade to the latest release of Cloudy (c08.00). However, you will have to upgrade to a newer g++ compiler, or...
Peter van Hoof
peter_van_hoof
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Sep 1, 2008
1:11 pm
581
Hi Gary and all cloudy folks! I downloaded the c08.00 version yesterday and try to run it on my IC418 model. I meet some problems... It seems that the label...
chris_morisset
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Sep 8, 2008
2:27 pm
582
Hi Christophe, He 2 7178A is the 11-5 transition. By default the new h-like He model (part of the new h-like isoelectronic sequence developed by myself) ...
rporter@...
ryan_l_porter
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Sep 8, 2008
9:28 pm
583
Hi everyone, I've been using Cloudy (version c08) to calculate the opacity of gas at various temperatures, densities, and metallicities. I am particularly...
Britton Smith
brittonsmith...
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Sep 15, 2008
8:50 pm
584
Hi there, this sounds like the protostellar disks problem. The code does not now include the chemistry that forms some molecules in a cold dust-free...
gary_ferland
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Sep 15, 2008
9:16 pm
585
Hi Britton, What you see at low energies is free-free opacity. This effect is dominated by hydrogen, which is why it is almost independent of metallicity. If...
Peter van Hoof
peter_van_hoof
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Sep 15, 2008
9:18 pm
586
Hi Gary and Peter, Thanks very much for responding to my question. The simulations I've been running are indeed without dust grains. I am mainly interested ...
Britton Smith
brittonsmith...
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Sep 16, 2008
3:25 pm
587
Hello, I'm confused about what the "set Lwidth" command does, and what is meant by "line width". I tried doing "set Lwidth 150,000km/s" and compared with "set...
lindastrubbe
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Sep 16, 2008
7:42 pm
588
Hi Linda, ... The code only adjusts the height of the line. It makes the implicit assumption that the line cannot be resolved due to the low resolution of the...
Peter van Hoof
peter_van_hoof
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Sep 16, 2008
8:43 pm
589
Thank you, Peter -- that's very helpful. Linda...
lindastrubbe
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Sep 18, 2008
6:34 pm
590
Hello, I managed to get a thrown assert using the turbulence command. Perhaps there's a maximum turbulent velocity -- the one I was using was very high....
lindastrubbe
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Sep 23, 2008
6:55 pm
591
Hi there, i ran the script with C08, the current release version, and it ended normally. you might try upgrading to the current version. good luck, Gary...
gary_ferland
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Sep 23, 2008
9:18 pm
592
Hello, I have been generating absorption models with Cloudy for xspec fitting, and am getting some strange results. I created the mtable model using the...
alexblustin
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Sep 25, 2008
4:58 pm
593
Hi Alex, check why the sims stopped. When the ionization parameter is high the gas was probably hot and the calculation extended to the requested stopping...
gary_ferland
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Sep 25, 2008
5:24 pm
594
Hello, Yes, the lowest ionisation calculations "stopped because lowest Te reached". So would it be best to run the simulations including cosmic rays, and...
Alex Blustin
alexblustin
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Sep 26, 2008
2:27 pm
595
... in nature the gas really would form molecules. so if you are after the absorption properties of a high column density molecular cloud then you should...
gary_ferland
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Sep 26, 2008
2:38 pm
596
Gary, Thanks for the information, I am now re-running the simulations as you suggested. Going through the output, I noticed another set of messages: NOTE...
Alex Blustin
alexblustin
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Sep 29, 2008
3:30 pm
597
Hi Alex, ... Yes, these are perfectly normal when using higher resolution. No need to be concerned. Peter. -- Peter van Hoof Royal Observatory of Belgium ...
Peter van Hoof
peter_van_hoof
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Sep 29, 2008
3:35 pm
598
Hi Cloudy folks, I noted a change since c08 in the Cloudy punch line output file that I don't really understand: c07: #Emission line structure. #depth H 1...
chris_morisset
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Oct 13, 2008
9:04 pm
599
hi! I have a problem with the emission lines. I check the lines ratios in the main output. It is supposed to print emergent lines intensities only on case of...
Ania Raiter
aniaraiter
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Oct 20, 2008
10:14 am
600
Hi Ania, this is a change between c07 and c08 - the emergent intensities were not predicted for a closed geometry in older versions, as you say. But we needed...
gary_ferland
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Oct 22, 2008
2:33 am
601
Hi Christophe, ... is this the output from the punch line emissivity command? it turned out that punch line emissivity and structure did the exact same thing...
gary_ferland
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Oct 22, 2008
2:50 am
602
hi! Gary,thanks for your answer, I tried the recent version of Cloudy and is all ok now. in the documentation it is only written that the distinction between...
Ania Raiter
aniaraiter
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Oct 22, 2008
10:03 am
603
Hi Gary, Thanks for your nice answer. The main problem with the format changes is that I have to ask for the Cloudy_3D users to define carefully which version...
chris_morisset
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Oct 24, 2008
7:43 pm
604
Hi Chris, which punch commands does the 3D code use? we could make sure that they don't change. There will probably be a service release in a month or two -...
gary_ferland
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Oct 25, 2008
1:08 am
605
... I use the followings: punch last cooling punch last heating punch last temperature punch last physical conditions punch last radius punch last continuum ...
chris_morisset
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Oct 25, 2008
4:53 am
606
Hi everyone! I am interested in calculating the ionization structure of very young and compact Hii regions. There are a number of very young Hii regions that...
djohan.vanderwalt01
djohan.vande...
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Nov 4, 2008
5:53 pm
607
... density. ... Cloudy approaches this problem from by doing the microphysics. So you would not set the electron density - that is determined by self ...
gary_ferland
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Nov 9, 2008
2:26 pm
608
I'm interested in producing a basic synthetic spectrum, like the one output in 'punch continuum' but higher resolution. I've read the Observed Quantities and...
g6.6742m11
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Nov 14, 2008
1:39 am
Messages 579 - 608 of 889   Oldest  |  < Older  |  Newer >  |  Newest
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