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Messages 58 - 89 of 486   Oldest  |  < Older  |  Newer >  |  Newest
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58
Hi, Gary, Nick, etc., I just have started using Cloudy to model my Spitzer data and of course, have a new question. How do I get Cloudy to print out the ...
erikandjan
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Dec 6, 2005
10:00 pm
59
... Hi Jan, I had never heard of these lines being detected. They are not in the code at the moment but the infrastructure is there to include them. Do you...
gary_ferland
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Dec 7, 2005
2:43 am
60
... Hi, Gary, Yes, we first detected these iron lines with the KAO, but unfortunately the only reference is to an AAS abstract by Erickson et al. (1989) (which...
erikandjan
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Dec 13, 2005
12:48 am
61
... et ... Ferland, ... proceeding ... ApJ, ... you ... Pradhan ... and ... and Hi Jan, by a bizarre coincidence, Kevin Blagrave added the lines and sent the...
gary_ferland
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Dec 13, 2005
1:00 am
62
Greetings, Release candidate 1 of C06.01, the next major version of Cloudy, is on the ftp site. To obtain this version go to the Cloudy / gold version page...
gary_ferland
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Jan 3, 2006
6:38 pm
63
Just thought I'd pass along my discovery that compiling Cloudy 05_07 with gcc version 4.0.2 (and I suspect 4.x) leads to problems if you use the...
jslavin37
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Feb 1, 2006
3:13 pm
64
Hello, I'm trying to model the dust thermal emission in a post-AGB nebula and I am wondering if there is a way of using the optimize command to reproduce a...
Carmen Sanchez Contre...
cscpasa
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Feb 2, 2006
2:44 pm
65
... and I am wondering ... color (e.g. the [12]-[25] ... you can optimize anything that is in the list of emission-line intensities, so the first step is to...
gary_ferland
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Feb 2, 2006
2:59 pm
66
Thanks for pointing this out! We did see these problems with icc 8.1 and adjusted our recommended icc compiler options in response. gcc 4.0.2 was not released...
peter_van_hoof
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Feb 9, 2006
6:34 pm
67
Dear Gary, I have somel questions about the output continuum files. I'm modeling the dust thermal emission from the circumstellar ennvelope around a post-AGB...
Carmen Sanchez Contre...
cscpasa
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Feb 9, 2006
7:36 pm
68
... above? The punch grain continuum command was added a very long time ago to enable debugging. It has the same units as the other punch continuum files but...
gary_ferland
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Feb 13, 2006
1:47 pm
69
Version 06.02 is now posted on the web site. Part 1 of Hazy and the Quick start guide have also been updated. Part 3 of Hazy is being updated and will be...
gary_ferland
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Feb 15, 2006
10:32 am
70
I'm wondering if you all are considering changing the Mg+ dielectronic recombination rates used in Cloudy. (By Mg+, I mean from Mg+ -> Mg0.) There are now two...
jslavin37
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Feb 15, 2006
5:45 pm
71
Dear CLOUDY developers and users, I have used CLOUDY in the past (until C96b4) to model fine structure lines spectra taken by ISO. Now I am very interested in...
Nemesio Rodriguez
nemesio_rf
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Feb 16, 2006
4:08 pm
72
Hi Nemesio, Thanks for your e-mail. The behavior with CO/C < 0.01 you noted when grain depletion is turned on does not seem unphysical given the temperature...
nicholas_p_abel
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Feb 16, 2006
6:47 pm
73
... (http://amdpp.phys.strath.ac.uk/tamoc/DR/) ... near ... The ... cases. I The default recombination rates in 06.02 remain unchanged. However the Badnell...
gary_ferland
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Feb 18, 2006
7:02 am
74
A new version of Part 3 of hazy is now posted on the code web site. Go to the documents folder of the current stable version. Good luck, Gary...
gary_ferland
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Feb 25, 2006
9:59 am
75
Hi Gary et al., A few papers (1,2,3) have recently found that the most up-to-date transition probability data for O+ (i.e., [O II] lines) may be incorrect....
kevin_blagrave
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Mar 6, 2006
10:07 pm
76
... the ... Cloudy ... to ... this ... Hi Kevin, is it possible to obtain a copy of your paper? how about posting on astro-ph - that was the first place I...
gary_ferland
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Mar 6, 2006
11:47 pm
78
... The paper should appear on astro-ph tonight. ... Thanks for the reference. We found that there was no noticeable difference between using old Pradhan or...
kevin_blagrave
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Mar 7, 2006
8:18 pm
79
Hi Gary, I am now trying to calculate some PDR models with the same parameters described in Abel et al. (2005, ApJS, 161, 65), using c06.02 (not c06.02a)....
tohru.nagao
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Mar 26, 2006
4:39 pm
80
Hi Tohru, your sim worked fine with 06.02a - Nick Abel had improved aspects of the ice formation physics. This is probably the source of the problem in 06.02...
gary_ferland
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Mar 26, 2006
11:23 pm
81
Greetings, Version 06.02a of Cloudy is posted on the web site www.nublado.org. This is a roll-up of all bug fixes we have made since 06.02 was released....
gary_ferland
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Mar 27, 2006
2:56 pm
82
Hi Gary, Thanks, I will try PDR calculations with 06.02a! regards, tohru...
tohru.nagao
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Mar 28, 2006
9:42 am
83
There is a new command that will allow the set of As to be selectred. This is in the development version and will become available in the next major release....
gary_ferland
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Mar 31, 2006
4:06 pm
84
What does the scale factor for table HM05 physically mean? Does it have some relation to the ionization parameter? In the past, it worked to set the...
Kathy Cooksey
klcooksey
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Apr 11, 2006
4:29 am
85
... have some relation to ... (to set the luminosity) and ... the shape). Now when I ... numbers of continuum ... Greetings You can still enter your own table...
gary_ferland
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Apr 11, 2006
11:23 am
87
Hi, I'm trying to get CLOUDY running to model some high redshift absorption line systems, and I got the error message shown below. Can anyone offer any advice...
ajfox279
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May 24, 2006
2:07 pm
88
... Hi there, I reproduced the problem here. It's a bug. I will let you know when there is a hotfix. thanks! Gary...
gary_ferland
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May 24, 2006
4:56 pm
89
the problem is that Li becomes so very highly ionized that its atomic abundance underflows to zero. The code detects the insanity and throws the assert. The...
gary_ferland
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May 24, 2006
8:38 pm
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