The pros and cons of the inversion method approach to...

Monthly Notices of the Royal Astronomical Society 2014 / 04 Vol. 440; Iss. 4

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 )

Traficante, A., Paladini, R., Compiegne, M., Alves, M. I. R., Cambresy, L., Gibson, S. J., Tibbs, C. T., Noriega-Crespo, A., Molinari, S., Carey, S. J., Ingalls, J. G., Natoli, P., Davies, R. D., Davi
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Volume:
440
Language:
english
Journal:
Monthly Notices of the Royal Astronomical Society
DOI:
10.1093/mnras/stu493
Date:
April, 2014
File:
PDF, 8.86 MB
english, 2014
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