Hello! Does anyone know about any publication regarding measurements and modelling (with cloudy) of the line HeI 1.083 micron in the context of AGNs/Seyfert...
Hi, Cristina. I was unable to find any such papers after some searching on the ADS, but I did find this 1978 paper by Feldman and MacAlpine entitled “A...
Dear Gary, Korista & Goad (2000) make use of the LOC model to interpret the BLR emission of ngc5548. In their fitting grid, they choose to limit the density to...
... above ... there are two high density limits - first is just the processor dealing with n^2 - for a 32 bit machine this limits the density to less than...
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 ...
... 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...
... 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...
... et ... Ferland, ... proceeding ... ApJ, ... you ... Pradhan ... and ... and Hi Jan, by a bizarre coincidence, Kevin Blagrave added the lines and sent the...
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...
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...
... 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...
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...
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...
... 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...
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...
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...
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...
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...
... (http://amdpp.phys.strath.ac.uk/tamoc/DR/) ... near ... The ... cases. I The default recombination rates in 06.02 remain unchanged. However the Badnell...
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....
... 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...
... 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...
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)....
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...
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....
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....
