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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