Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust
- Collaboration, Planck
- Adam, R.
- Ade, R.
- Aghanim, N.
- Alves, R.
- Arnaud, M.
- Arzoumanian, D.
- Ashdown, M.
- Aumont, J.
- Baccigalupi, C.
- Banday, J.
- Barreiro, R.
- Bartolo, N.
- Battaner, E.
- Benabed, K.
- Benoit-Lévy, A.
- Bersanelli, M.
- Bielewicz, P.
- Bonaldi, A.
- Bonavera, L.
- Bond, R.
- Borrill, J.
- Bouchet, R.
- Boulanger, F.
- Bracco, A.
- Burigana, C.
- Butler, R.
- Calabrese, E.
- Cardoso, J.
- Catalano, A.
- Chamballu, A.
- Chiang, C.
- Christensen, R.
- Colombi, S.
- Colombo, P.
- Combet, C.
- Couchot, F.
- Crill, P.
- Curto, A.
- Cuttaia, F.
- Danese, L.
- Davies, R.
- Davis, R.
- Bernard, P.
- de Rosa, A.
- de Zotti, G.
- Delabrouille, J.
- Dickinson, C.
- Diego, M.
- Dole, H.
- Donzelli, S.
- Doré, O.
- Douspis, M.
- Ducout, A.
- Dupac, X.
- Efstathiou, G.
- Elsner, F.
- Ensslin, A.
- Eriksen, K.
- Falgarone, E.
- Ferrière, K.
- Finelli, F.
- Forni, O.
- Frailis, M.
- Fraisse, A.
- Franceschi, E.
- Frejsel, A.
- Galeotta, S.
- Galli, S.
- Ganga, K.
- Ghosh, T.
- Giard, M.
- Gjerløw, E.
- González-Nuevo, J.
- Górski, M.
- Gregorio, A.
- Gruppuso, A.
- Guillet, V.
- Hansen, K.
- Hanson, D.
- Harrison, D.
- Henrot-Versillé, S.
- Hernández-Monteagudo, C.
- Herranz, D.
- Hildebrandt, R.
- Hivon, E.
- Hobson, M.
- Holmes, A.
- Hovest, W.
- Huffenberger, M.
- Hurier, G.
- Jaffe, A.
- Jaffe, R.
- Jones, C.
- Juvela, M.
- Keihänen, E.
- Keskitalo, R.
- Kisner, S.
- Kneissl, R.
- Knoche, J.
- Kunz, M.
- Kurki-Suonio, H.
- Lagache, Guilaine
- Lamarre, M.
- Lasenby, A.
- Lattanzi, M.
- Lawrence, R.
- Leonardi, R.
- Levrier, F.
- Liguori, M.
- Lilje, P.
- Linden-Vørnle, M.
- López-Caniego, M.
- Lubin, P.
- Macias-Perez, J.
- Maffei, B.
- Maino, D.
- Mandolesi, N.
- Maris, M.
- Marshall, D.
- Martin, P.
- Martínez-González, E.
- Masi, S.
- Matarrese, S.
- Mazzotta, P.
- Melchiorri, A.
- Mendes, L.
- Mennella, A.
- Migliaccio, M.
- Miville-Deschênes, M.
- Moneti, A.
- Montier, L.
- Morgante, G.
- Mortlock, D.
- Munshi, D.
- Murphy, J.
- Naselsky, P.
- Natoli, P.
- Nørgaard-Nielsen, H.
- Noviello, F.
- Novikov, D.
- Novikov, I.
- Oppermann, N.
- Oxborrow, C.
- Pagano, L.
- Pajot, F.
- Paoletti, D.
- Pasian, F.
- Perdereau, O.
- Perotto, L.
- Perrotta, F.
- Pettorino, V.
- Piacentini, F.
- Piat, M.
- Plaszczynski, S.
- Pointecouteau, E.
- Polenta, G.
- Ponthieu, N.
- Popa, L.
- Pratt, G.
- Prunet, S.
- Puget, J.
- Rachen, P.
- Reach, T.
- Reinecke, M.
- Remazeilles, M.
- Renault, C.
- Ristorcelli, I.
- Rocha, G.
- Roudier, G.
- Rubiño-Martín, J.
- Rusholme, B.
- Sandri, M.
- Santos, D.
- Savini, G.
- Scott, D.
- Soler, D.
- Spencer, D.
- Stolyarov, V.
- Sudiwala, R.
- Sunyaev, R.
- Sutton, D.
- Suur-Uski, A.
- Sygnet, J.
- Tauber, J.
- Terenzi, L.
- Toffolatti, L.
- Tomasi, M.
- Tristram, M.
- Tucci, M.
- Umana, G.
- Valenziano, L.
- Valiviita, J.
- van Tent, B.
- Vielva, P.
- Villa, Francesca
- Wade, A.
- Wandelt, D.
- Wehus, K.
- Wiesemeyer, H.
- Yvon, D.
- Zacchei, A.
- Zonca, A.
DOIAbstract
International audienceThe role of the magnetic field in the formation of the filamentary structures observed in the interstellar medium (ISM) is a debated topic. The Planck all-sky maps of linearly polarized emission from dust at 353GHz provide the required combination of imaging and statistics to study the correlation between the structures of the Galactic magnetic field and of interstellar matter, both in the diffuse ISM and in molecular clouds. The data reveal structures, or ridges, in the intensity map with counterparts in the Stokes Q and/or U maps. We focus on structures at intermediate and high Galactic latitudes with column density from 1020 to 1022 cm−2. We measure the magnetic field orientation on the plane of the sky from the pol...
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