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The pros and cons of the inversion method approach to derive 3D dust emission properties of the ISM: the Hi-GAL field centred on (l,b)=(30,0)
Alessio Traficante, Roberta Paladini, Mathieu Compiegne +13
Herschel FIR continuum data obtained as part of the Hi-GAL survey have been used, together with the GLIMPSE 8 m and MIPSGAL 24 m data, to attempt the first 3D-decomposition o…
Spitzer IRS Detection of Molecular Hydrogen Rotational Emission Towards Translucent Clouds
James G. Ingalls, T. M. Bania, F. Boulanger +3
Using the Infrared Spectrograph on board the Spitzer Space Telescope, we have detected emission in the S(0), S(1), and S(2) pure-rotational (v=0-0) transitions of molecular hydroge…
C in Reflection Nebulae
Kris Sellgren, Michael W. Werner, James G. Ingalls +3
The fullerene C has four infrared-active vibrational transitions at 7.0, 8.5, 17.4 and 18.9 m. We have previously observed emission features at 17.4 and 18.9 m in the…