Astronomy and Astrophysics – Astronomy
Scientific paper
May 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103..461p&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, May 1991, p. 461-467.
Astronomy and Astrophysics
Astronomy
35
Molecular Clouds, Protostars, Radio Astronomy, Radio Telescopes, Signal Processing, Spiral Galaxies, Galactic Nuclei, Infrared Astronomy Satellite, Spectral Bands
Scientific paper
The telescopes and signal processing systems of the Owens Valley Millimeter Array are considered, and improvements in the sensitivity and stability of the instrument are characterized. The instrument can be applied to map sources in the 85 to 115 GHz and 218 to 265 GHz bands with a resolution of about 1 arcsec in the higher frequency band. The operation of the array is fully automated. The current scientific programs for the array encompass high-resolution imaging of protoplanetary/protostellar disk structures, observations of molecular cloud complexes associated with spiral structure in nearby galaxies, and observations of molecular structures in the nuclei of spiral and luminous IRAS galaxies.
Finch R. P.
Giovanine C. J.
Lawrence Ronald P.
Padin Stephen
Scott Susannah L.
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