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| Author |
Kaeufl, H. U.; Rothermel, H.; Drapatz, S. |
| Title |
Indication for H2O in the upper atmosphere of Mars |
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Journal Article |
| Year |
1984 |
Publication |
Astron. Astrophys. |
Abbreviated Journal |
A&A |
| Volume |
141 |
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430-432 |
| Keywords |
atmospheric moisture, mars atmosphere, upper atmosphere, water vapor, carbon dioxide, emission spectra, nonequilibrium thermodynamics, polar regions |
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452 |
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Rothermel, H.; Käufl, H. U.; Yu, Y. |
| 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 |
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Pages |
387-392 |
| Keywords |
astronomical spectroscopy, infrared astronomy, infrared spectrometers, optical heterodyning, infrared telescopes, laser spectrometers, mars (planet), venus (planet) |
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453 |
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| Author |
Tokunaga, Alan T. |
| Title |
High resolution infrared spectroscopy of planetary atmospheres |
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Journal Article |
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1983 |
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Astron. Soc. Pacific. Pub. |
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95 |
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691-699 |
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454 |
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Betz, A. L.; Johnson, M. A.; McLaren, R. A.; Sutton, E. C. |
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Heterodyne detection of CO2 emission lines and wind velocities in the atmosphere of Venus |
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Journal Article |
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1976 |
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Astrophys. J. |
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208 |
Issue |
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Pages |
L141-L144 |
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carbon dioxide, emission spectra, optical heterodyning, planetary radiation, venus atmosphere, wind velocity, doppler effect, infrared radiation, ultraviolet radiation, venus clouds |
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455 |
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Hansen, Lene; Jørgensen, H.E.; Nørgaard-Nielsen, Hans Ulrik; Pedersen, Kenneth; Goudfrooij, P.; Linden-Vornle, M.J.D. |
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ISO far-infrared observations of rich galaxy clusters III. Abell 2029, Abell 2052, Abell 2142 |
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2000 |
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Astron. Astrophys. |
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A&A |
| Volume |
362 |
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1 |
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133-137 |
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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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RPLAB @ s @ |
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456 |
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