Published in
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 )
Journal article published in 2014 by
A. Traficante 
,
R. Paladini,
M. Compiegne,
M. I. R. Alves,
L. Cambresy,
S. J. Gibson,
C. T. Tibbs,
A. Noriega-Crespo,
S. Molinari ,
S. J. Carey ,
J. G. Ingalls,
P. Natoli,
R. D. Davies,
R. J. Davis,
C. Dickinson
and other authors.
,
R. Paladini,
M. Compiegne,
M. I. R. Alves,
L. Cambresy,
S. J. Gibson,
C. T. Tibbs,
A. Noriega-Crespo,
S. Molinari ,
S. J. Carey ,
J. G. Ingalls,
P. Natoli,
R. D. Davies,
R. J. Davis,
C. Dickinson
and other authors.
This paper was not found in any repository, but could be made available legally by the author.
Full text: Unavailable
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