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Sub-millimeter to centimeter excess emission from the Magellanic Clouds. I. Global spectral energy distribution
F. P. Israel, W. F. Wall, D. Raban +5
In order to reconstruct the global SEDs of the Magellanic Clouds over eight decades in spectral range, we combined literature flux densities representing the entire LMC and SMC res…
Herschel photometry of brightest cluster galaxies in cooling flow clusters
A. C. Edge, J. B. R. Oonk, R. Mittal +24
The dust destruction timescales in the cores of clusters of galaxies are relatively short given their high central gas densities. However, substantial mid-infrared and sub-mm emiss…
Herschel observations of FIR emission lines in brightest cluster galaxies
A. C. Edge, J. B. R. Oonk, R. Mittal +24
The question of how much gas cools in the cores of clusters of galaxies has been the focus of many, multiwavelength studies in the past 30 years. In this letter we present the firs…
The Distribution and Condition of the Warm Molecular Gas in Abell 2597 and Sersic 159-03
J. B. R. Oonk, W. Jaffe, M. N. Bremer +1
We have used the SINFONI integral field spectrograph to map the near-infrared K-band emission lines of molecular and ionised hydrogen in the central regions of two cool core galaxy…