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Messages 598 - 627 of 888   Oldest  |  < Older  |  Newer >  |  Newest
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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
609
... column ... Sorry - this is embarrassing, but my code was converting from Rydbergs to Angstroms incorrectly. So ignore the 1580A break thing. I'm still not...
g6.6742m11
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Nov 14, 2008
3:02 am
610
... i am not sure what you are after - but if it is just the sed at high resolution couldn't you just increase the resolution with the SET RESOLUTION command?...
gary_ferland
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Nov 18, 2008
3:28 pm
611
... high ... are ... for it. Do you mean 'set continuum resolution'? (I can't find any 'set resolution' command described.) Hazy says the 'punch continuum' ...
g6.6742m11
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Nov 18, 2008
10:23 pm
612
... doesn't ... to ... To be more clear, my questions are: 1. What continuua are used in 'punch continuum'? No 'punch X continuum' command I've tried gives me...
g6.6742m11
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Nov 18, 2008
10:32 pm
613
... yes, set continuum resolution. sorry. the format of the wavelength is a small bug. most of the wavelengths are given with .5e format. The punch...
gary_ferland
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Nov 20, 2008
11:48 am
614
... you looked at the figure on page 145 of hazy 1? ... they should be the same since there are just a few vectors being output in different places. can you...
gary_ferland
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Nov 20, 2008
12:15 pm
615
Hi photoionized folks! I wonder if there is an easy way to add a user-defined ionizing continuum that would not suffer dilution with the distance to the center...
chris_morisset
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Nov 25, 2008
7:58 pm
616
Thanks for the tip on editing punch_do.cpp. Thanks also for patiently working through these basics with me. ... Yes, but this is tied to my apparent result...
g6.6742m11
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Nov 26, 2008
9:28 pm
617
Hi! During an optimization with Phymir method (for a Planetary Nebula) Cloudy 08.00 has done this errors: Iteration 16 Chisq= 8.21076e+03 ...
patrizia.manzitto
patrizia.man...
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Nov 27, 2008
10:20 am
618
Hi Patrizia, It seems that you are using a user-defined density law (DLAW call in the input file). To reproduce the problem one will need this function, which...
chris_morisset
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Nov 27, 2008
4:23 pm
619
Hi Patrizia, Christophe is right. We do need the contents of the file dense_fabden.cpp in order to be able to investigate this problem. Also, could you try...
Peter van Hoof
peter_van_hoof
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Nov 28, 2008
3:56 pm
620
... this is underway but won't be done anytime soon. Plans are in place and all it will take is a few weeks of work. But our attention has been focused on...
gary_ferland
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Nov 28, 2008
3:59 pm
621
Hi Patrizia, I have found an old fabden that I sent to you, and with that I could exactly reproduce the problem on c08_branch, but not the trunk. This is the...
Peter van Hoof
peter_van_hoof
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Nov 28, 2008
4:29 pm
622
... Hi Gary, thanks for the answer. Do you think then that changing a mano the haardt_madau_galaxy.dat file would do the job? I don't care the molecules, just...
chris_morisset
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Nov 28, 2008
6:01 pm
623
Hello, I've been using cloudy (c07.02.02) for a short while, but since attempting to use a source continuum calculated externally (input via the interpolate...
timbob4242
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Dec 9, 2008
1:33 pm
624
... the "trans" is the emission you would see if the cloud were directly along our line of sight. You see a huge damped La line and a strong CI absorption...
gary_ferland
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Dec 10, 2008
1:28 pm
625
Hello, I am using the release version C08.00. I ran a series of models optimized to a line ratio. I also included 4 punched ...
pellegriniew
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Dec 10, 2008
3:34 pm
626
Hello, I'm trying to apply Cloudy c08.00 to Bania Clump 1 and Clump 2 in the Inner Galaxy, but am unsure of the kind of input I should use. I have 12CO J7-6,...
wickedboconan
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Dec 12, 2008
2:51 am
627
Hi, Sorry, I was going to edit my post rather than post again, but wasn't able to find a way to do that. I decided that my description of the problem was...
timbob4242
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Dec 12, 2008
1:43 pm
Messages 598 - 627 of 888   Oldest  |  < Older  |  Newer >  |  Newest
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