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Messages 859 - 888 of 888   Oldest  |  < Older  |  Newer >  |  Newest
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859
Thanks Ryan!...
Andrea
a_ruff
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Oct 7, 2009
9:12 pm
860
Hi Peter, Thank you for your help. I use the "interpolate" and "intensity" commands to make it work. Thanks again, Yangsen...
Yangsen
yangseny
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Oct 7, 2009
11:42 pm
861
Hi Bert, The problem is that the interpolate is expecting the log of the energy in Rydbergs or, confusingly, the log of the frequency for numbers greater than...
Ryan L Porter
ryan_l_porter
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Oct 9, 2009
11:50 pm
862
Hi, I have a new level2.dat file, with the 6 main FeXVII transitions included and updated. All the data are from CHIANTI, including the collision strengths...
burkinafaso76
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Oct 12, 2009
12:43 pm
863
Hi Stefano, ... Sure, anything that improves the data in Cloudy is welcome! Peter. ... -- Peter van Hoof Royal Observatory of Belgium Ringlaan 3 1180 Brussel ...
Peter van Hoof
peter_van_hoof
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Oct 13, 2009
10:50 am
864
The updated level2.dat file is in the 'Files' section. Let me know if it is ok and if you need more detailed comments for the changes. Stefano...
burkinafaso76
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Oct 13, 2009
12:43 pm
865
Hi all, I use phymir optimization method for the modeling of planetary nebulae SEDs. Sometimes even if i set 500 iterations, phymir stop the procedure before...
patrizia.manzitto
patrizia.man...
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Oct 13, 2009
1:03 pm
866
Hi Patrizia, My first comment is that you do not have enough observables. You have 3 observables to constrain 4 parameters, that can never work. To make...
Peter van Hoof
peter_van_hoof
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Oct 13, 2009
3:10 pm
867
Hi, I'm a bit confused by the labels of the O II 3727 line. If I interpret them correctly, IONZ 3727A is radiative recombination (both lines) O II 3729A is...
valentina_viridiana
valentina_vi...
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Oct 19, 2009
12:02 pm
868
Hi Valentina there is a PUNCH LINE LABELS command which gives the ID, wavelength, and a brief comment explaining the line. here are the [O II] entries in C08:...
Gary Ferland
gary_ferland
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Oct 19, 2009
7:59 pm
869
Hi Gary, yes, it is precisely those labels I find obscure, e.g.: - I don't get the meaning of "line produced by photoionization of Oo" - I understand from the...
Valentina Luridiana
valentina_vi...
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Oct 20, 2009
11:16 am
870
... the process is described in 1986PASP...98..549F for C lines, in 1981ApJ...244.1022F for [O II], and in AGN3 on page 38. ... the above process....
Gary Ferland
gary_ferland
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Oct 20, 2009
5:48 pm
871
Hello, Can anyone walk me through how to check the ionizing photon flux from a punch incident continuum? I'm working with the HM05 background spectrum at z=0,...
emehrinker
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Oct 24, 2009
11:16 pm
872
Hi all, I'm confused about the right way to go about the pumping part of Hbeta. I'm computing models without pumping in three different ways (with "no induced...
valentina_viridiana
valentina_vi...
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Oct 25, 2009
3:30 pm
873
Hi, ... correct. ... All you need to do is divide nuJnu by the photon energy, which is given in infinite mass Rydberg (R_inf). See section 3.5 of Hazy 3. Then...
Peter van Hoof
peter_van_hoof
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Oct 26, 2009
12:17 pm
874
Hey, I have been messing around with different abundances and ran across an interesting issue. Using element scale factor works great for every element I've...
coldfir1784
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Oct 28, 2009
11:41 pm
875
Hi Bert,       According the Hazy, the Cloudy-preferred spelling of that element is "Sulphur" (Table 16).  I don't know which is the "correct" spelling...
Rajib Ganguly
ganguly2001
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Oct 28, 2009
11:52 pm
876
Hi again, it seems this message has gone unnoticed. Any help? Thanks, Valentina...
valentina_viridiana
valentina_vi...
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Oct 29, 2009
9:46 pm
877
Hey all, I have a more difficult question than I have asked in the past which goes more to the heart of how cloudy works. I want to input my own abundance...
coldfir1784
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Oct 29, 2009
10:15 pm
878
... they should all agree, and should all be zero. so i am confused too. ... a quick look at the source suggests that your original interpretation should be...
Gary Ferland
gary_ferland
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Nov 1, 2009
3:01 am
879
Hi Bert, Rajib, Rajib is correct. The preferred spelling in Cloudy is "sulphur", which is the British spelling, and the US spelling "sulfur" is not recognized....
Peter van Hoof
peter_van_hoof
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Nov 1, 2009
12:54 pm
880
Hello, I was wondering if there is a way to have Cloudy punch the absorption opacities of lines as a function of depth in the cloud. I'm looking for something...
lindastrubbe
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Nov 2, 2009
10:20 pm
881
Hi Linda, I hope somebody will correct me if I'm wrong, but I don't think Cloudy has a command for that, at least not yet. But, I was once interested in the...
John Everett
everett@...
Send Email
Nov 3, 2009
3:26 pm
882
Hi Bert, Yes, you can specify abundances relative to hydrogen that are greater than unity. There are several such models in the test suite. One example is...
Ryan L Porter
ryan_l_porter
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Nov 4, 2009
12:19 am
883
Hi John, Thanks for your reply. I think for the moment, I've found a way to approximately calculate what I need well enough without that command. But I might...
lindastrubbe
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Nov 4, 2009
5:56 pm
884
Hi there, I was looking over the 'table stars' command, and it wasn't completely clear to me whether there are input spectra only for single stars or for SSPs...
wiersmarp
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Nov 6, 2009
1:36 pm
885
Hi Rob, You can use Starburst99 and PopStar SSPs at least. See the wiki: http://wiki.nublado.org/wiki/StellarAtmospheres Cheers, Jarle....
Jarle Brinchmann
jarlebrinchmann
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Nov 8, 2009
12:34 am
886
Hi Rob, Alternatively, if neither Starburst99 or PopStar suit your needs, you can fairly easily incorporate other grids by making your own .ascii file. A full...
Peter van Hoof
peter_van_hoof
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Nov 8, 2009
2:05 pm
887
Hello, I have recently started using cloudy and am now trying to use it to model the effect of a blackhole binary on the environment. I am using an incident...
dhuppenkothen
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Nov 9, 2009
12:19 pm
888
Hi there, it is getting the right answer - the radio brightness temperature is VERY large. make a plot of the incident radiation field with data from the...
Gary Ferland
gary_ferland
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Nov 9, 2009
8:25 pm
Messages 859 - 888 of 888   Oldest  |  < Older  |  Newer >  |  Newest
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