Mathematics – Logic
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20922303n&link_type=abstract
2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #223.03; Bulletin of the American Astronomical Society,
Mathematics
Logic
1
Scientific paper
Recent pioneering CO observations of infrared luminous galaxies and AGN at high-z allow us to study coevolution of black hole growth and star formation in galaxies during the heydey of massive galaxy formation. However, little is known concerning the physical nature of these crucial galaxies, and the relationship between the central AGN, ISM, and host galaxy properties to the observed CO emission. In order to provide a framework for an interpretation of these observations, I investigate the nature of the CO emission in starburst galaxies and quasars by combining a 3D non-LTE radiative transfer code with cosmological and galaxy merger hydrodynamic simulations. Here, I highlight recent results from these simulations. Specifically, I will discuss the following: 1. The effect of black hole growth and starbursts on CO emission patterns; 2. The role of galactic winds on CO emission morphologies and line profiles; 3. The nature of CO emission in z 6 Quasars, and how we might use this to constrain models of primordial galaxy formation.
Chakrabarti Sangeeta
Cox Tom
Dav'e Romeel
Di Matteo Tiziana
Hernquist Lars
No associations
LandOfFree
Models of the Molecular Interstellar Medium in Starbursts and AGN from z=0-6 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 Models of the Molecular Interstellar Medium in Starbursts and AGN from z=0-6, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Models of the Molecular Interstellar Medium in Starbursts and AGN from z=0-6 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1164333