Proposal code
v037
Proposal title
Extragalactic OH Masers
The |
Investigators and their |
Affiliations |
P.I. |
Karl M. Menten |
Harvard-Smithsonian CfA |
|
Lincoln J. Greenhill |
Harvard-Smithsonian CfA |
|
James M. Moran |
Harvard-Smithsonian CfA |
|
Mark J. Reid |
Harvard-Smithsonian CfA |
Proposal Abstract
We propose VSOP observations to map the two strongest
OH megamasers Arp 220 and III Zw 35.
Many important questions remain to be answered concerning
the nature of these ``megamaser" galaxies.
Of central importance is the question of the relation
between of the OH maser emission and the active nuclei in these systems.
Some models suggest that the masers are low-gain amplifiers and
arise from regions at distances of a few hundred pc from the galactic nuclei,
while recent transatlantic VLBI observations of Arp 220 indicate high-gain
maser emission, with the bulk of the emission being emitted from a region
smaller than 1 pc. Through VSOP maps of these two megamasers, we hope
to obtain sufficient angular resolution to settle this controversy,
to spatially resolve the OH velocity field, and to determine the
enclosed masses in these systems.
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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
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Also note that AO1 proposals were submitted in November 1995, and information such
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may therefore have changed.