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Author Chen, P. S. url  doi
openurl 
  Title Infrared properties of barium stars Type Journal Article
  Year 2001 Publication Astron. Astrophys. Abbreviated Journal A&A  
  Volume 372 Issue 1 Pages 245-248  
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  ISSN 0004-6361 ISBN Medium  
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  Notes Approved no  
  Call Number RPLAB @ s @ Serial 415  
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Author Omar, A.; Anantharamaiah, K. R.; Rupen, M.; Rigby, J. url  doi
openurl 
  Title VLA detection of OH absorption from the elliptical galaxy NGC 1052 Type Journal Article
  Year 2002 Publication Astron. Astrophys. Abbreviated Journal A&A  
  Volume 381 Issue 1 Pages L29-L32  
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  Notes Approved no  
  Call Number RPLAB @ s @ Serial 435  
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Author Kawamura, J.; Hunter, T. R.; Tong, C. Y. E.; Blundell, R.; Papa, D. C.; Patt, F.; Peters, W.; Wilson, T.; Henkel, C.; Goltsman, G.; Gershenzon, E. url  doi
openurl 
  Title Ground-based terahertz CO spectroscopy towards Orion Type Journal Article
  Year 2002 Publication A&A Abbreviated Journal A&A  
  Volume 394 Issue 1 Pages 271-274  
  Keywords HEB mixers, applications  
  Abstract Using a superconductive hot-electron bolometer heterodyne receiver on the 10-m Heinrich Hertz Telescope on Mount Graham, Arizona, we have obtained velocity-resolved 1.037 THz CO () spectra toward several positions along the Orion Molecular Cloud (OMC-1) ridge. We confirm the general results of prior observations of high-J CO lines that show that the high temperature, , high density molecular gas, , is quite extended, found along a ~ region centered on BN/KL. However, our observations have significantly improved angular resolution, and with a beam size of we are able to spatially and kinematically discriminate the emission originating in the extended quiescent ridge from the very strong and broadened emission originating in the compact molecular outflow. The ridge emission very close to the BN/KL region appears to originate from two distinct clouds along the line of sight with and ≈ . The former component dominates the emission to the south of BN/KL and the latter to the north, with a turnover point coincident with or near BN/KL. Our evidence precludes a simple rotation of the inner ridge and lends support to a model in which there are multiple molecular clouds along the line of sight towards the Orion ridge.  
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  Call Number Serial 322  
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Author Käufl, H. U.; Rothermal, H.; Drapatz, S. openurl 
  Title Investigation of the Martian atmosphere by 10 micron heterodyne spectroscopy Type Journal Article
  Year 1984 Publication Astron. Astrophys. Abbreviated Journal A&A  
  Volume 136 Issue Pages 319-325  
  Keywords astronomical spectroscopy, atmospheric composition, infrared astronomy, mars atmosphere, spectral line width, carbon dioxide concentration, nonequilibrium thermodynamics, optical heterodyning, planetary radiation, mars, atmosphere, spectroscopy, atmosphere, carbon dioxide, altitude, kinetics, rotation, thermal properties, temperature, emissions, intensity, models, data, spectra  
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  Call Number Serial 449  
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Author Rothermel, H.; Käufl, H. U.; Schrey, U.; Drapatz, S. openurl 
  Title Thermal structure of the Martian mesosphere Type Journal Article
  Year 1988 Publication Astron. Astrophys. Abbreviated Journal A&A  
  Volume 196 Issue Pages 296-300  
  Keywords atmospheric temperature, carbon dioxide, infrared spectroscopy, mars atmosphere, mesosphere, emission spectra, line spectra, spatial resolution, mars, atmosphere, mesosphere, structure, thermal properties, spectra, spectroscopy, earth-based observations, temperature, patterns, infrared, polar regions, wavelengths, equipment, procedure, carbon dioxide, emissions  
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  Notes Approved no  
  Call Number Rothermel1988 Serial 450  
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