Comparison of 13CO line and far-infrared continuum emission as a diagnostic of dust and molecular gas physical conditions - II. The simulations: testing the method

Monthly Notices of the Royal Astronomical Society

Volumn 377, Issue 2, 2007, Pages 545-555

  Wall, W F ^a  

^a INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

Author keywords

Dust, extinction; ISM: molecules

Indexed keywords

DENSITY OF GASES; SPECTROSCOPY;

CO LINE; CONTINUUM EMISSION; DUST EXTINCTIONS; FAR INFRARED; INFRARED: CONTINUUM; ISM:MOLECULES; MOLECULAR GAS; ORDERS OF MAGNITUDE; PHYSICAL CONDITIONS; SPECTRAL LINE;

DUST;

EID: 34247575188     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11566.x     Document Type: Article

References (4)

1. COBE Diffuse Infrared Background Experiment (DIRBE) Explanatory Supplement, 1998, in Hauser M. G., Kelsall T., Leisawitz D., Weiland J., eds, version 2.3, COBE Ref. Pub. 98-A. NASA/GSFC, Greenbelt, MD (available in electronic form from the NSSDC)
2. Nagahama T., Mizuno A., Ogawa H., Fukui Y., 1998, AJ, 116, 336
3. Wall W. F., 2007a, MNRAS, 375, 278 (Paper I)
4. Wall W. F., 2007b, MNRAS, in press (doi : Paper III, this issue)