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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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  ISSN 0004-6361 ISBN Medium  
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  Notes Approved no  
  Call Number RPLAB @ s @ Serial 435  
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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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  Notes Approved no  
  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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Author Johnson, M. A.; Betz, A. L.; McLaren, R. A.; Townes, C. H.; Sutton, E. C. openurl 
  Title Nonthermal 10 micron CO2 emission lines in the atmospheres of Mars and Venus Type Journal Article
  Year 1976 Publication Astron. Astrophys. Abbreviated Journal A&A  
  Volume 208 Issue Pages 145  
  Keywords carbon dioxide, emission spectra, infrared spectra, mars atmosphere, nonthermal radiation, optical heterodyning, planetary radiation, venus atmosphere, absorption spectra, energy transfer, line spectra, molecular absorption, molecular collisions, near infrared radiation, solar flux  
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  Notes Approved no  
  Call Number ref1976ApJ...208L.145J Serial 451  
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Author Kaeufl, H. U.; Rothermel, H.; Drapatz, S. openurl 
  Title Indication for H2O in the upper atmosphere of Mars Type Journal Article
  Year 1984 Publication Astron. Astrophys. Abbreviated Journal A&A  
  Volume 141 Issue Pages 430-432  
  Keywords atmospheric moisture, mars atmosphere, upper atmosphere, water vapor, carbon dioxide, emission spectra, nonequilibrium thermodynamics, polar regions  
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  Notes Approved no  
  Call Number Serial 452  
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Author Rothermel, H.; Käufl, H. U.; Yu, Y. openurl 
  Title A heterodyne spectrometer for astronomical measurements at 10 micrometers Type Journal Article
  Year 1983 Publication Astron. Astrophys. Abbreviated Journal A&A  
  Volume 126 Issue Pages 387-392  
  Keywords astronomical spectroscopy, infrared astronomy, infrared spectrometers, optical heterodyning, infrared telescopes, laser spectrometers, mars (planet), venus (planet)  
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  Notes Approved no  
  Call Number Serial 453  
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Author Hansen, Lene; Jørgensen, H.E.; Nørgaard-Nielsen, Hans Ulrik; Pedersen, Kenneth; Goudfrooij, P.; Linden-Vornle, M.J.D. openurl 
  Title ISO far-infrared observations of rich galaxy clusters III. Abell 2029, Abell 2052, Abell 2142 Type Journal Article
  Year 2000 Publication Astron. Astrophys. Abbreviated Journal A&A  
  Volume 362 Issue 1 Pages 133-137  
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  Abstract A sample of five rich galaxy clusters has been mapped by ISO at 60 μm, 100 μm, 135 μm, and 200 μm using the PHT-C camera. In previous papers Abell 2670 and Sersic 159-03 were discussed. Here we present the results for Abell 2029, Abell 2052, and Abell 2142. The conclusion of the survey is that the relatively small fields (approximate to 60 square are minutes) are structured with filaments or superpositions of point sources. In some cases point sources (approximate to 0.1 Jy) can be identified with cluster galaxies. An attempt to demonstrate infrared emission from dust in the cooling flows (due to star formation) was inconclusive.  
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  Call Number RPLAB @ s @ Serial 456  
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Author Bruderer, S.; Benz, A. O.; van Dishoeck, E. F.; Melchior, M.; Doty, S. D.; van der Tak, F.; Stäuber, P.; Wampfler, S. F.; Dedes, C.; Yıldız, U. A.; Pagani, L.; Giannini, T.; de Graauw, Th.; Whyborn, N.; Teyssier, D.; Jellema, W.; Shipman, R.; Schieder, R.; Honingh, N.; Caux, E.; Bächtold, W.; Csillaghy, A.; Monstein, C.; Bachiller, R.; Baudry, A.; Benedettini, M.; Bergin, E.; Bjerkeli, P.; Blake, G. A.; Bontemps, S.; Braine, J.; Caselli, P.; Cernicharo, J.; Codella, C.; Daniel, F.; di Giorgio, A. M.; Dominik, C.; Encrenaz, P.; Fich, M.; Fuente, A.; Goicoechea, J. R.; Helmich, F.; Herczeg, G. J.; Herpin, F.; Hogerheijde, M. R.; Jacq, T.; Johnstone, D.; Jørgensen, J. K.; Kristensen, L. E.; Larsson, B.; Lis, D.; Liseau, R.; Marseille, M.; McCoey, C.; Melnick, G.; Neufeld, D.; Nisini, B.; Olberg, M.; Parise, B.; Pearson, J. C.; Plume, R.; Risacher, C.; Santiago-García, J.; Saraceno, P.; Shipman, R.; Tafalla, M.; van Kempen, T. A.; Visser, R.; Wyrowski, F. doi  openurl
  Title Herschel/HIFI detections of hydrides towards AFGL 2591. Envelope emission versus tenuous cloud absorption Type Journal Article
  Year 2010 Publication Astron. Astrophys. Abbreviated Journal  
  Volume 521 Issue Pages L44 (1 to 7)  
  Keywords HEB mixer applications, HIFI, Herschel  
  Abstract The Heterodyne Instrument for the Far Infrared (HIFI) onboard the Herschel Space Observatory allows the first observations of light diatomic molecules at high spectral resolution and in multiple transitions. Here, we report deep integrations using HIFI in different lines of hydrides towards the high-mass star forming region AFGL 2591. Detected are CH, CH+, NH, OH+, H2O+, while NH+ and SH+ have not been detected. All molecules except for CH and CH+ are seen in absorption with low excitation temperatures and at velocities different from the systemic velocity of the protostellar envelope. Surprisingly, the CH(JF,P = 3/22,- – 1/21,+ ) and CH+(J = 1–0, J = 2–1) lines are detected in emission at the systemic velocity. We can assign the absorption features to a foreground cloud and an outflow lobe, while the CH and CH+ emission stems from the envelope. The observed abundance and excitation of CH and CH+ can be explained in the scenario of FUV irradiated outflow walls, where a cavity etched out by the outflow allows protostellar FUV photons to irradiate and heat the envelope at larger distances driving the chemical reactions that produce these molecules.  
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  Call Number Serial 1083  
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Author Soifer, B. T.; Pipher, J. L. url  doi
openurl 
  Title Instrumentation for infrared astronomy Type Journal Article
  Year 1978 Publication Annual Rev. Astron. Astrophys. Abbreviated Journal  
  Volume 16 Issue 1 Pages 335-369  
  Keywords infrared applications  
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  Series Volume Series Issue (up) Edition  
  ISSN 0066-4146 ISBN Medium  
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  Notes Approved no  
  Call Number Serial 492  
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