Proposal code
w050
Proposal title
Cores of Lobe-dominated Quasars with VSOP - Epoch 2
The |
Investigators and their |
Affiliations |
P.I. |
R.W.Porcas |
MPIfR, Bonn, GERMANY |
|
J.A.Zensus |
MPIfR, Bonn, GERMANY |
|
D.H.Hough |
Trinity University, San Antonio, TX, USA |
Proposal Abstract
The study of the parsec-scale morphology and kinematics of quasars
is central to the understanding of extragalactic radio source jet
physics, and the classification of various types of objects. In
the "unified schemes" the
properties of sources should depend crucially upon the angle of a
relativistically moving plasma with respect to the
line of sight. Core-dominated sources should
show properties corresponding to an axis nearly pointing at the
observer - superluminal motion, exaggeration of small bends,
and strong and variable cores. In contrast, in lobe-
dominated quasars these properties should be weak or absent.
We wish to make SECOND EPOCH VSOP OBSERVATIONS of our small sample of
LOBE-DOMINATED QUASARS, to compare the sub-mas structures and component
velocities
with those of the stronger core-dominated
quasars. Our sources are at high declinations, and are thus ideal
for efficient use of VSOP-GRT time.
The full Cover Sheets
(compressed post-script, typically 50kbytes) can
be retrieved. Note that many proposals were reduced in extent by the
Scientific Review Committee (e.g. by reducing the number of
experiments), however the Cover Sheets contain the full proposal as
submitted. Also note that AO2 proposals were submitted in May 1998,
and information such as affiliations and contact details has
changed for some proposers since that time. The Cover Sheets (and the
details on this page, which were derived from the Cover Sheets) may
therefore have changed.