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Infrared to millimetre photometry of ultra-luminous IR galaxies: new evidence favouring a 3-stage dust model

U. Klaas·M. Haas·S. A. H. Mueller·R. Chini·B. Schulz·I. Coulson·H. Hippelein·K. Wilke·M. Albrecht·D. Lemke
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Abstract

Infrared to millimetre spectral energy distributions have been obtained for 41 bright ultra-luminous infrared galaxies. The observations were carried out with ISOPHOT between 10 and 200 micron and supplemented for 16 sources with SCUBA at 450 and 850 micron and with SEST at 1.3 mm. In addition, seven sources were observed at 1.2 and 2.2 $μ$m with the 2.2 m telescope on Calar Alto. These new SEDs represent the most complete set of infrared photometric templates obtained so far on ULIRGs in the local universe.

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U. Klaas, M. Haas, S. A. H. Mueller, R. Chini, B. Schulz, I. Coulson, H. Hippelein, K. Wilke, M. Albrecht, D. Lemke. 2001-10-09. Infrared to millimetre photometry of ultra-luminous IR galaxies: new evidence favouring a 3-stage dust model. https://doi.org/10.1051/0004-6361%3A20011377

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