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1.
The Hi-GAL compact source catalogue – I. The physical properties of the clumps in the inner Galaxy (−71$_{.}^{\circ}$0 < ℓ < 67$_{.}^{\circ}$0) / Elia, Davide (INAF, Rome) ; Molinari, S. (INAF, Rome) ; Schisano, E. (INAF, Rome) ; Pestalozzi, M. (INAF, Rome) ; Pezzuto, S. (INAF, Rome) ; Merello, M. (INAF, Rome) ; Noriega-Crespo, A. (Baltimore, Space Telescope Sci.) ; Moore, T.J. T. (Liverpool John Moores U., ARI) ; Russeil, D. (Marseille, Lab. Astrophys.) ; Mottram, J.C. (Heidelberg, Max Planck Inst. Astron.) et al.
Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 $\mu$m. We present a band-merged catalogue of spatially matched sources and their properties derived from fits to the spectral energy distributions (SEDs) and heliocentric distances, based on the photometric catalogs presented in Molinari et al. [...]
arXiv:1706.01046.- 2017 - 44 p. - Published in : Mon. Not. R. Astron. Soc. 471 (2017) 100-143 Fulltext: PDF;
2.
Spatial distribution of star formation related to ionized regions throughout the inner Galactic plane / Palmeirim, P. (Marseille, Lab. Astrophys. ; Porto U., Astron. Dept.) ; Zavagno, A. (Marseille, Lab. Astrophys.) ; Elia, D. (INAF, Rome) ; Moore, T.J. T. (Liverpool John Moores U., ARI) ; Whitworth, A. (Cardiff U.) ; Tremblin, P. (MdlS, Saclay) ; Traficante, A. (INAF, Rome) ; Merello, M. (INAF, Rome) ; Russeil, D. (Marseille, Lab. Astrophys.) ; Pezzuto, S. (INAF, Rome) et al.
We present a comprehensive statistical analysis of star-forming objects located in the vicinities of 1 360 bubble structures throughout the Galactic Plane and their local environments. The compilation of ~70 000 star-forming sources, found in the proximity of the ionized (Hii) regions and detected in both Hi-GAL and GLIMPSE surveys, provided a broad overview of the different evolutionary stages of star-formation in bubbles, from prestellar objects to more evolved young stellar objects (YSOs). [...]
arXiv:1705.09877.- 2017-09-05 - 14 p. - Published in : Astron. Astrophys. 605 (2017) A35 Fulltext: PDF;
3.
Planck 2013 results. XIII. Galactic CO emission / Planck collaboration
Rotational transition lines of CO play a major role in molecular radio astronomy and in particular in the study of star formation and the Galactic structure. Although a wealth of data exists in the Galactic plane and some well-known molecular clouds, there is no available CO high sensitivity all-sky survey to date. [...]
arXiv:1303.5073; CERN-PH-TH-2013-126; CERN-PH-TH-2013-126.- 2014-10-29 - 22 p. - Published in : Astron. Astrophys. 571 (2014) A13 Fulltext: PDF; External links: Preprint; EDP Sciences Free Access article

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