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Article
A Search for Variability in the HCCN to H2CO Ratio in Comet Hale-Bopp
We observed submillimeter lines of H2CO and HCN in comet Hale-Bopp near perihelion. One of our goals was to search for short term variability. Our observations are suggestive, but not conclusive, of temporal and/...
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Chapter and Conference Paper
CO (3-2) Observations of Spiral Galaxies
We report the detection of the CO J=3-2 line in several nearby galaxies, including M82, M83, and NGC 253. The line intensities indicate that the nuclear gas in these galaxies is very warm (T≳ 30–50K), and ofte...
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Chapter and Conference Paper
Submillimeter Instrument Development at Steward Observatory
Receiver instrumentation for the UA/MPIfR Submillimeter Telescope (SMT) is being assured through three different mechanisms. (1) There will be standard facility instruments. Initially, these include 460 GHz an...
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Chapter and Conference Paper
The SMT: A Joint Submillimeter Telescope Project of the Mar-Planck-Institut für Radioastronomie and Steward Observatory
We present a summary of the main features of the SMT project with emphasis on the site and the organisational aspects. Technical features of the telescope are presented in the proceedings of the Zermatt Sympos...
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Chapter and Conference Paper
CO J=2-1 Observations Toward Southern HII Regions
A spectral line receiver system developed at the Max-Planck-Institut für Radioastronomie in Bonn was installed on the ESO 3.6 m and 1 m telescopes in July 1981. The cooled mixer frontend gave DSB receiver temp...
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Chapter and Conference Paper
Small Scale Clum** in the Orion Molecular Cloud
The results of new maps of the Orion Molecular Cloud in lines of NH3 and H2CO are presented. The angular resolution of these maps varies from 1’ (for the 211 – 212 line of H2CO at 14.5 GHz, using the 100-m telesc...