Physics
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..783..123a&link_type=abstract
THE EVOLUTION OF STARBURSTS: The 331st Wilhelm and Else Heraeus Seminar. AIP Conference Proceedings, Volume 783, pp. 123-134 (2
Physics
Galaxies, Galactic Nuclei, Interstellar Matter, Gases, Star Formation, Starburst Galaxies And Infrared Excess Galaxies, Galactic Nuclei, Circumnuclear Matter, And Bulges, Atomic, Molecular, Chemical, And Grain Processes, Origin, Formation, Evolution, Age, And Star Formation
Scientific paper
Understanding the molecular phase of the ISM in starburst and active galaxies is important for the modelling of the onset and evolution of their nuclear activity. Here, we focus on single dish and high resolution studies of 12CO and 13CO and how to use the 12CO/13CO 1-0 line intensity ratio as a diagnostic tool for large scale ISM properties in galaxies.
Observations of high density gas tracers like HCN, HNC, HC3N, HCO+ and CN are essenatial for probing physical and chemical conditions of the dense, star-forming gas. These tracers show great potential as indicators of the evolution of star formation as well as probes of X-ray illuminated molecular gas around and active galactic nucleus.
No associations
LandOfFree
Probing Molecular Gas Properties in Starbursts and AGNs does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Probing Molecular Gas Properties in Starbursts and AGNs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Probing Molecular Gas Properties in Starbursts and AGNs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1344998