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Title
We present the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key program that will map the inner Galactic plane of the Milky Way in 5 bands. We outline our data reduction strategy and present some science high...
We present the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key program that will map the inner Galactic plane of the Milky Way in 5 bands. We outline our data reduction strategy and present some science high...
Molinari, S.;Swinyard, B.;Bally, J.;Barlow, M.;Bernard, J.-P.;Martin, P.;Moore, T.;Noriega-Crespo, A.;Plume, R.;Testi, L.;Zavagno, A.;Abergel, A.;Ali, B.;Anderson, L.;André, P.;Baluteau, J.-P.;Battersby, C.;Beltrán, M. T.;Benedettini, M.;Billot, N.;Blommaert, J.;Bontemps, S.;Boulanger, F.;Brand, J.;Brunt, C.;Burton, M.;Calzoletti, L.;Carey, S.;Caselli, P.;Cesaroni, R.;Cernicharo, J.;Chakrabarti, S.;Chrysostomou, A.;Cohen, M.;Compiegne, M.;de Bernardis, P.;de Gasperis, G.;di Giorgio, A. M.;Elia, D.;Faustini, F.;Flagey, N.;Fukui, Y.;Fuller, G. A.;Ganga, K.;Garcia-Lario, P.;Glenn, J.;Goldsmith, P. F.;Griffin, M.;Hoare, M.;Huang, M.;Ikhenaode, D.;Joblin, C.;Joncas, G.;Juvela, M.;Kirk, J. M.;Lagache, G.;Li, J. Z.;Lim, T. L.;Lord, S. D.;Marengo, M.;Marshall, D. J.;Masi, S.;Massi, F.;Matsuura, M.;Minier, V.;Miville-Deschênes, M.-A.;Montier, L. A.;Morgan, L.;Motte, F.;Mottram, J. C.;Müller, T. G.;Natoli, P.;Neves, J.;Olmi, L.;Paladini, R.;Paradis, D.;Parsons, H.;Peretto, N.;Pestalozzi, M.;Pezzuto, S.;Piacentini, F.;Piazzo, L.;Polychroni, D.;Pomarès, M.;Popescu, C. C.;Reach, W. T.;Ristorcelli, I.;Robitaille, J.-F.;Robitaille, T.;Rodón, J. A.;Roy, A.;Royer, P.;Russeil, D.;Saraceno, P.;Sauvage, M.;Schilke, P.;Schisano, E.;Schneider, N.;Schuller, F.;Schulz, B.;Sibthorpe, B.;Smith, H. A.;Smith, M. D.;Spinoglio, L.;Stamatellos, D.;Strafella, F.;Stringfellow, G. S.;Sturm, E.;Taylor, R.;Thompson, M. A.;Traficante, A.;Tuffs, R. J.;Umana, G.;Valenziano, L.;Vavrek, R.;Veneziani, M.;Viti, S.;Waelkens, C.;Ward-Thompson, D.;White, G.;Wilcock, L. A.;Wyrowski, F.;Yorke, H. W.;Zhang, Q.
We present the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key program that will map the inner Galactic plane of the Milky Way in 5 bands. We outline our data reduction strategy and present some science high...
We use the13CO (2-1) emission from the SEDIGISM (Structure, Excitation, and Dynam-ics of the Inner Galactic InterStellar Medium) high-resolution spectral-line survey of the innerGalaxy, to extract the molecular cloud population with a large dynamic r...
By combining two surveys covering a large fraction of the molecular material in the Galactic disk we investigate the role the spiral arms play in the star formation process. We have matched clumps identified by ATLASGAL with their parental GMCs as id...