Proposal code
w401
Proposal title
Structural variablity in the brightest AGN: AO 0235+164
The |
Investigators and their |
Affiliations |
P.I. |
S. Frey |
F\"OMI SGO, Hungary |
|
L.I. Gurvits, D.C. Gabuzda |
JIVE, The Netherlands |
|
D.R. Altschuler, C.J.Salter, P. Perillat |
NAIC Arecibo, Puerto Rico |
|
H.D. Aller, M.F. Aller |
U. Michigan RAO, USA |
|
H. Hirabayashi |
ISAS, Japan |
|
M.M. Davis |
SETI Institute, USA |
Proposal Abstract
AO 0235+164 is a very compact, violently variable BL Lac object. Our earlier 5-GHz VSOP
observation (v040b, 1 Feb 1999) revealed a compact core with the brightness temperature
in excess of 5.8\times10^{13} K (the highest value measured with VSOP to date)
and a weak extension on sub-mas scale.
We request time to enhance the earlier VSOP result on this source.
The high dynamic range, 1.6 and 5-GHz polarisation monitoring observations
proposed here could reveal structural
changes on time scales of 2 weeks and 6 months. Supporting ground-based monitoring
observations are planned to investigate the connection between the possible
sub-mas scale structural, total and polarized radio flux density, and spectral variations,
exactly at the same epochs as of the VSOP observations proposed.
The full Cover Sheets
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Scientific Review Committee (e.g. by reducing the number of
experiments), however the Cover Sheets contain the full proposal as
submitted. Also note that AO4 proposals were submitted in October 2000,
and information such as affiliations and contact details has
changed for some proposers since that time.