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Messages 623 - 652 of 888   Oldest  |  < Older  |  Newer >  |  Newest
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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
628
Hi Everett, Here are a number of thoughts on your question: -Allow optically thick results (by replacing your "stop zone 1" command with a "stop column density...
Ryan Porter
ryan_l_porter
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Dec 12, 2008
10:52 pm
629
hi Tim, several things - you are a major mod behind on the cloudy version - we are at C08. we try to have the major version agree with the year so that it is...
gary_ferland
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Dec 16, 2008
3:25 am
630
Hello Everett, I have done a bit of work on using cloudy to model molecular lines. I have also had trouble matching the level populations of 12CO in the Orion...
pellegriniew
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Dec 16, 2008
10:34 pm
631
... *** High resolution X-ray spectroscopy: towards IXO *** ** Spectroscopy workshop 19-20 March 2009 ** ** Spectroscopy school 17-18 March 2009 ** UCL Mullard...
alexblustin
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Dec 22, 2008
10:07 am
632
Hi Ryan, Thank you for your wealth of suggestions. I have also uploaded our modifications to the constants for CO in atmdat_lines_setup.cpp in the Files...
wickedboconan
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Dec 24, 2008
4:04 am
633
Hi Everett, I'm glad to hear you've had some success. Thanks for uploading your data. We'll look into it after we complete the upgrade to the LAMDA data. ...
Ryan Porter
ryan_l_porter
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Dec 30, 2008
11:14 pm
634
hi, i am trying to get Cloudy to output (punch) data which will allow me to make a plot of how the ionization states of a few ions varies with radius - the...
jamesfurness@...
jamesfurness...
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Jan 8, 2009
4:55 pm
635
sorry, i have since found it. typical....
jamesfurness@...
jamesfurness...
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Jan 8, 2009
5:13 pm
636
Hi Eric, At the AAS meeting you mentioned that turbulence can be an important source of heating and indeed Clump 1 and Clump 2 in the Inner Galaxy are highly...
wickedboconan
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Jan 22, 2009
8:18 pm
637
Hi Everett, I would be happy to help you set up a model. We talked about a lot of different things at AAS including turbulence but you should check with the...
pellegriniew
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Jan 26, 2009
7:12 am
638
hi! I have a problem with N4 line 1486A. This is a doublet 1485+1486 actually. If I check the lines intensities and ratios in the main output .out they are...
Ania Raiter
aniaraiter
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Jan 27, 2009
1:30 pm
639
Hi Anna, this is indeed a bug. To fix it change lines 662 & 663 of prt_lines_lv1_li_ne.cpp from linadd(embesq.em1486,1485,"N 4",'i', " the N 4] slow...
gary_ferland
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Jan 27, 2009
11:33 pm
640
... Hi Peter and Christophe, I apologize if I write only now in the discussion board!!! I use this "dense_fabden.cpp" that I wrote below; in that file I wrote ...
patrizia.manzitto
patrizia.man...
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Jan 28, 2009
4:12 pm
641
 Hi,  I am interested in the heating and cooling rates for a gas with arbitrary density, temperature and metallicty. Without dust, a gas of solar...
Yafo Escasibar
yascasibar
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Jan 28, 2009
4:42 pm
642
Hi Yago, yes, this result makes sense. Collisions between gas and grains will tend to bring the temperatures of the two together. If you do a simulation that...
gary_ferland
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Jan 29, 2009
5:12 pm
643
Hi Yafo, I completely agree with Gary's response. The first question you have to ask is whether the presence of grains in a 10 MK plasma is realistic. What is...
Peter van Hoof
peter_van_hoof
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Jan 29, 2009
11:39 pm
644
Hello there, I was wondering if there's an easy way to simulate a plasma of a given density that is in LTE at a single given temperature (not externally...
lindastrubbe
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Jan 30, 2009
7:26 am
645
Hi Linda, Yes, indeed. The simplest way to do this would be something like the following: hden 4 coronal 4 init "honly.ini" stop zone 1 The ³coronal²...
Ryan Porter
ryan_l_porter
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Jan 30, 2009
8:07 am
646
Hi, First of all, thank you very much for your explanations. I must confess I was not originally interested in such a hot gas, but I think this result, if...
yascasibar
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Jan 30, 2009
1:49 pm
647
Hi there, One empirical way to see if grains are present is to look for gas-phase depletions. In the galactic ISM elements like Ca, Al, and Fe are strongly...
gary_ferland
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Jan 30, 2009
2:36 pm
648
Hi Linda, My response was less than helpful for a few reasons. Firstly, my example doesn¹t come close to reaching LTE. Secondly, I didn¹t even address your...
Ryan Porter
ryan_l_porter
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Jan 30, 2009
8:48 pm
649
Hi Ryan, Thanks for your replies! I tried your first suggestion this morning and was slowly coming to the conclusion that I wasn't in LTE, so thanks for...
lindastrubbe
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Jan 31, 2009
2:53 am
650
Hi Eric, I have been searching for observed turbulent velocities, but have been unable to find any. I believe they are difficult to estimate because the...
wickedboconan
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Jan 31, 2009
5:06 am
651
Hi Linda, Yes, you could lower the density, add whatever SED you like, and increase the ionization parameter until you have enough photons to achieve LTE at ...
Ryan Porter
ryan_l_porter
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Jan 31, 2009
7:05 pm
652
Hi Everet, The turbulent velocities should be in km/s but the constants in the equations I mentioned before convert the heating to to cgs units. Maybe now...
pellegriniew
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Jan 31, 2009
8:00 pm
Messages 623 - 652 of 888   Oldest  |  < Older  |  Newer >  |  Newest
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