: |
: |
|---|
D. N. FRIEDEL, L. E. SNYDER, University of Illinois, Dept. of Astronomy, 1002 W. Green St, Urbana, IL 61801; B. E. TURNER, National Radio Astronomy Observatory, Charlottesville, VA 22903; ANTHONY J. REMIJAN, NASA Goddard Space Flight Center, Space and Earth Data Computing Division, Code 930, Greenbelt, MD 20771; National Research Council Resident Research Associate.
With the Berkeley-Illinois-Maryland-Association (BIMA) Array we have carried out a 3 mm (80-115.9 GHz) spectral line survey of Orion-KL. Orion-KL is composed of several distinct regions separated by only a few arcseconds, most notably the ``Hot Core'', where N bearing species are most prevalent, and the ``Compact Ridge'', where O bearing species are most prevalent. For our observations the average synthesized beam was 14''x8''. We detected over 700 spectral features from the ``Hot Core'' and over 600 spectral features from the ``Compact Ridge''. We will present the abundances and spatial distribution of the detected species.