Primeval galaxies in the sub-mm and MM

Details Primeval galaxies in the sub-mm and MM Primeval galaxies in the sub-mm and MM

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf...21b&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 21-22 (SEE N93-26706 10-90)

Astronomy and Astrophysics

Astronomy

3

Astronomical Models, Black Body Radiation, Cosmic Background Explorer Satellite, Millimeter Waves, Radio Astronomy, Radio Galaxies, Submillimeter Waves, Interferometers, Telescopes

Scientific paper

Although the results of COBE's FIRAS experiment 1 constrain the deviation in energy from the CMB blackbody in the 500-5000 micron range to be delta E/E, sub cmb less than 0.005, primeval galaxies can still lead to a brilliant sub-mm sky of non-Gaussian sources that are detectable at 10 inch resolution from planned arrays such as SCUBA on the James Clerk Maxwell Telescope and, quite plausibly, at sub-arcsecond resolution in planned mm and sub-mm interferometers. Here, we apply our hierarchical peaks method to a CDM model to construct sub-mm and mm maps of bursting PG's appropriate for these instruments with minimum contours chosen to correspond to realistic observational parameters for them and which pass the FIRAS limits.

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