K. C. Chambers
Published 1998-11-11Version 1
The continuum morphologies of high redshift radio galaxies and quasars can be modeled as enormous bipolar reflection nebulae from shells of dust swept up by bipolar outflows. If the observed shape of a particular object is fit with an analytic function, then the velocity of the shell is specified by the equations of motion. The predicted kinematics can be compared with the observed emission line velocity field, and the resulting fit is excellent. The implications for massive galaxies at high redshift include the requirement of an initial epoch of star formation that creates dust distributed throughout a very large, diffuse, nearly virialized halo.
Comments: To appear in ``After the Dark Ages: When Galaxies Were Young'', Ninth Annual October Astrophysics Conference in Maryland, ed. S. S. Holt and E. P. Smith, (New York: American Institute of Physics Press), 1998
Spitzer Observations of High Redshift Radio Galaxies
Dust in High Redshift Radio Galaxies and the Early Evolution of Spheroidal Galaxies
The Morphology of HII Galaxies
