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....
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...
... 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...
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...
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...
Hi photoionizing folks! The Cloudy_3D webserver is open at http://132.248.1.102/Cloudy_3D You can download there papers on NEBU_3D (the precursor of C3D) and...
I'm new to Cloudy, and go the error: "Sorry, Something bad has happened." I was wondering if there is someone who can help me with why this is happening....
... The root cause was the combination of galactic cosmic rays and the very low gas density. The density is roughly four orders of magnitude lower than the...
