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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 4(440), p. 3588-3612, 2014

DOI: 10.1093/mnras/stu493

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The pros and cons of the inversion method approach to derive 3D dust emission properties in the ISM: the Hi-GAL field centred on (l, b) = (30 , 0 )

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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