- ...densities.
-
Sources that are optically thick at 43 GHz will have higher
proportions of their total flux in an unresolved core at 86
GHz, while those that are optically thin at 43 GHz should
have about the same fraction in the core at 86 GHz as at 43
GHz.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1998).
-
Note that observed brightness temperatures are reduced by a
factor of (1+z) from the brightness temperatures in
the source co-moving frames; at a typical blazar redshift of
z=1, the brightness temperature at the source redshift
would need to be 29#29 K in order to yield an observed value
of 30#30 K.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...redshifts.
-
Note that this list contains several gravitationally lensed
sources; no attempt has been made to account for the fact
that lensing permits better intrinsic resolution in those
objects.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
Connect with NRAO