... goals are to: 1) investigate the di#erences in physical characteristics (velocity width, HI mass, etc.) for sources with AGN's and those with pure starbursts; 2) study the OH gas properties, especially the occurrence of masers and activity in the OH ...
[
Текст
]
Ссылки http://www.naic.edu/vscience/schedule/tpfiles/ZauderertagA2361tp.ps -- 96.5 Кб -- 09.10.2007 Похожие документы
... It is the focus of considerable attention in the search for unambiguous evidence of starburst or AGN activity, in order to shed light on the ultimate origin of the quasar-like bolometric luminosity, and on the possibility of an evolutionary sequence ...
... halo Resimulate most massive halo (1015M at z=0) to derive merger tree Hydrodynamically simulate galaxy mergers Formulation for AGN feeback and starburst winds Non-LTE Radiative Transfer · · Monte Carlo Code Subgrid formalism for mass spectrum of GMCs ...
[
Текст
]
Ссылки http://www.naic.edu/~astro/chicago2/talks/Narayanan-CO_Emissionin_high-z_QSOs.pdf -- 735.5 Кб -- 21.08.2006 Похожие документы
... p.4/17 Intergalactic & Intracluster Fields Only upper limits on a pervasive intergalactic field Evidence for turbulent amplification of cluster fields Interaction of magnetic fields & cosmic rays with AGN Are accretion shocks magnetized & how far back ...
... fo cus of my research has b een the application of radio astronomical techniques to the studies of Active Galactic Nuclei (AGN) and their hosts, the inter-galactic medium as seen via absorption lines against compact radio sources, and the magneto-ionic ...
... The VSOP 5 GHz AGN Survey I. Compilation and Observations". 2000, PASJ, 52, 997. ... 1) Atomic and Molecular Gas in AGN Hosts: Interactions b etween AGNs and their hosts ...
... eastern nucleus of this double-nuclear starburst galaxy, in which the western comp onent has b een considered to harb or an AGN ... 26. Hirabayashi et al., " The VSOP 5 GHz AGN Survey I. Compilation and Observations", 2000, PASJ, 52, 997. 27. ...