Planck intermediate results XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust
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G. W. Pratt | P. A. R. Ade | J. Aumont | S. Masi | N. Ponthieu | J. R. Bond | L. Toffolatti | F. Pasian | B. P. Crill | W. A. Holmes | G. Savini | J. D. Soler | W. Hovest | A. Catalano | M. Frailis | J. Borrill | A. Gruppuso | E. Hivon | L. Montier | G. Morgante | P. Natoli | F. Piacentini | M. Remazeilles | F. Cuttaia | L. Terenzi | O. Dor'e | M. Maris | S. Galeotta | M. Bersanelli | C. Burigana | N. Mandolesi | S. Plaszczynski | E. Pointecouteau | B. Maffei | L. Pagano | W. C. Jones | V. Stolyarov | G. Polenta | F. Pajot | I. Ristorcelli | F. Perrotta | V. Guillet | S. R. Hildebrandt | C. A. Oxborrow | A. Moneti | D. Santos | H. K. Eriksen | C. Dickinson | A. J. Banday | C. R. Lawrence | A. Mennella | P. B. Lilje | D. Herranz | D. L. Harrison | B. D. Wandelt | E. Falgarone | J.-F. Cardoso | K. Ganga | I. K. Wehus | N. Oppermann | D. Hanson | G. Lagache | L. Bonavera | P. Vielva | N. Aghanim | X. Dupac | J. P. Rachen | A. Zacchei | D. Maino | L. Perotto | M. Douspis | J. F. Mac'ias-P'erez | J. Delabrouille | S. Matarrese | L. Valenziano | A. Benoit-L'evy | A. Zonca | T. S. Kisner | E. Calabrese | M. Arnaud | M. Tomasi | A. H. Jaffe | O. Forni | K. Ferriere | F. Levrier | H. C. Chiang | S. Donzelli | F. Couchot | D. J. Marshall | F. Boulanger | P. M. Lubin | D. Novikov | P. Mazzotta | A. Gregorio | R. B. Barreiro | B. Rusholme | D. Scott | A. Ducout | C. Renault | D. Munshi | R. Keskitalo | E. Franceschi | L. Danese | C. Baccigalupi | L. Mendes | H. U. Norgaard-Nielsen | J. M. Diego | G. Hurier | M. Lattanzi | W. T. Reach | M. Kunz | H. Kurki-Suonio | V. Pettorino | L. Popa | F. Pasian | L. Valenziano | H. Kurki-Suonio | P. Lilje | N. Aghanim | C. Baccigalupi | K. Benabed | M. Kunz | G. Morgante | M. Douspis | M. Frailis | A. Zacchei | S. Colombi | A. Melchiorri | V. Pettorino | J. Rubino-Mart'in | O. Forni | T. Ensslin | E. Hivon | A. Banday | F. Hansen | M. Reinecke | A. Lasenby | B. Wandelt | F. Bouchet | S. Matarrese | P. Ade | J. Borrill | P. Bernardis | A. Jaffe | J. Bond | B. Crill | K. Ganga | W. Jones | S. Masi | F. Piacentini | S. Prunet | G. Efstathiou | J. Diego | A. Benoit-Lévy | A. Gregorio | M. Ashdown | C. Lawrence | B. Rusholme | R. Davis | T. Kisner | T. Jaffe | H. Eriksen | F. Couchot | S. Plaszczynski | W. Reach | F. Boulanger | H. Nørgaard-Nielsen | R. Davies | C. Dickinson | M. Arnaud | J. Aumont | E. Battaner | J. Bernard | M. Bersanelli | P. Bielewicz | A. Bonaldi | L. Bonavera | C. Burigana | R. C. Butler | A. Catalano | A. Chamballu | H. Chiang | L. Colombo | A. Curto | F. Cuttaia | L. Danese | A. Rosa | G. Zotti | J. Delabrouille | H. Dole | S. Donzelli | O. Dor'e | X. Dupac | E. Falgarone | F. Finelli | A. Fraisse | E. Franceschi | S. Galeotta | M. Giard | J. Gonz'alez-Nuevo | K. M. G'orski | A. Gruppuso | D. Hanson | D. Harrison | S. Henrot-Versill'e | C. Hern'andez-Monteagudo | D. Herranz | S. Hildebrandt | W. Holmes | W. Hovest | K. Huffenberger | E. Keihanen | R. Keskitalo | R. Kneissl | J. Knoche | G. Lagache | J. Lamarre | R. Leonardi | M. Liguori | M. Linden-Vørnle | M. L'opez-Caniego | P. Lubin | J. Mac'ias-P'erez | B. Maffei | D. Maino | N. Mandolesi | M. Maris | D. Marshall | P. Martin | E. Mart'inez-Gonz'alez | P. Mazzotta | L. Mendes | A. Mennella | M. Migliaccio | M. Miville-Deschênes | A. Moneti | L. Montier | D. Mortlock | D. Munshi | P. Naselsky | P. Natoli | F. Noviello | D. Novikov | I. Novikov | L. Pagano | F. Pajot | D. Paoletti | O. Perdereau | L. Perotto | F. Perrotta | M. Piat | E. Pointecouteau | G. Polenta | N. Ponthieu | L. Popa | G. Pratt | J. Puget | J. Rachen | M. Remazeilles | C. Renault | I. Ristorcelli | G. Rocha | G. Roudier | M. Sandri | D. Santos | G. Savini | L. Spencer | R. Sudiwala | R. Sunyaev | D. Sutton | A. Suur-Uski | J. Sygnet | J. Tauber | L. Terenzi | L. Toffolatti | M. Tomasi | M. Tristram | M. Tucci | G. Umana | J. Valiviita | B. Tent | P. Vielva | F. Villa | L. Wade | I. Wehus | D. Yvon | A. Zonca | E. Calabrese | F. Elsner | S. Galli | E. Gjerløw | M. Lattanzi | J. Murphy | V. Stolyarov | N. Bartolo | J. Cardoso | C. Combet | A. Ducout | A. Frejsel | T. Ghosh | G. Hurier | F. Levrier | N. Oppermann | J. Soler | M. Alves | A. Bracco | Planck Collaboration R. Adam | K. Ferrière | D. Arzoumanian | V. Guillet | H. Wiesemeyer | A. Bonaldi | F. Villa | M. Sandri | M. Ashdown | N. Bartolo | K. Benabed | J.-P. Bernard | P. Bielewicz | F. R. Bouchet | A. Bracco | L. P. L. Colombo | C. Combet | A. Curto | R. J. Davis | P. de Bernardis | A. de Rosa | G. de Zotti | G. Efstathiou | F. Elsner | T. A. Ensslin | F. Finelli | A. A. Fraisse | S. Galli | T. Ghosh | M. Giard | J. Gonz'alez-Nuevo | F. K. Hansen | E. Keihanen | J.-M. Lamarre | A. Lasenby | M. Liguori | M. L'opez-Caniego | P. G. Martin | E. Mart'inez-Gonz'alez | A. Melchiorri | M. Migliaccio | M.-A. Miville-Deschenes | P. Naselsky | D. Paoletti | O. Perdereau | J.-L. Puget | M. Reinecke | G. Rocha | G. Roudier | J. A. Rubino-Mart'in | A.-S. Suur-Uski | J. A. Tauber | M. Tristram | J. Valiviita | P. R. Christensen | E. Battaner | A. Chamballu | S. Colombi | R. D. Davies | H. Dole | K. M. Huffenberger | T. R. Jaffe | R. Kneissl | J. Knoche | R. Leonardi | D. Mortlock | J. A. Murphy | F. Noviello | I. Novikov | M. Piat | S. Prunet | L. D. Spencer | R. Sudiwala | R. Sunyaev | D. Sutton | J.-F. Sygnet | M. Tucci | B. Van Tent | L. A. Wade | D. Yvon | H. Wiesemeyer | S. Henrot-Versill'e | C. Hern'andez-Monteagudo | M. Linden-Vornle | G. Umana | M. I. R. Alves | A. Frejsel | E. Gjerlow | D. Arzoumanian | D. Scott | P. Christensen | D. Scott | J. Murphy | D. Scott | G. Rocha | J. Murphy | J. Bond | D. Harrison | C. Lawrence | D. Marshall | A.-S. Suur-Uski
[1] R. F. Loewenstein,et al. Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds , 2006 .
[2] Analysis of spiral arms using anisotropic wavelets: gas, dust and magnetic fields in M51 , 2006, astro-ph/0609787.
[3] F. O. Alves,et al. Optical polarimetry toward the Pipe nebula: revealing the importance of the magnetic field , 2008, 0806.1189.
[4] S. Masi,et al. First detection of polarization of the submillimetre diffuse galactic dust emission by Archeops , 2003, astro-ph/0306222.
[5] P. Koch,et al. MAGNETIC FIELD PROPERTIES IN HIGH-MASS STAR FORMATION FROM LARGE TO SMALL SCALES: A STATISTICAL ANALYSIS FROM POLARIZATION DATA , 2010, 1008.0220.
[6] Enrico Fermi,et al. Magnetic fields in spiral arms , 1953 .
[7] E. Ostriker,et al. DENSE CORE FORMATION IN SUPERSONIC TURBULENT CONVERGING FLOWS , 2011, 1101.2650.
[8] A. Lazarian,et al. Astrophysical Hydromagnetic Turbulence , 2013, 1307.5496.
[9] Christopher F. McKee,et al. THE DARK MOLECULAR GAS , 2010, 1004.5401.
[10] L. Hartmann,et al. Rapid Formation of Molecular Clouds and Stars in the Solar Neighborhood , 2001, astro-ph/0108023.
[11] T. Maciaszek,et al. Planck pre-launch status: The HFI instrument, from specification to actual performance , 2010 .
[12] N. Peretto,et al. Herschel view of the Taurus B211/3 filament and striations: evidence of filamentary growth? , 2012, 1211.6360.
[13] P. Hennebelle,et al. The structure of the thermally bistable and turbulent atomic gas in the local interstellar medium , 2013, 1301.3446.
[14] J. Kerp,et al. Dark matter in the Milky Way II. The HI gas distribution as a tracer of the gravitational potential , 2007, 0704.3925.
[15] Tsuyoshi Inoue,et al. TWO-FLUID MAGNETOHYDRODYNAMICS SIMULATIONS OF CONVERGING H i FLOWS IN THE INTERSTELLAR MEDIUM. II. ARE MOLECULAR CLOUDS GENERATED DIRECTLY FROM A WARM NEUTRAL MEDIUM? , 2009, 0908.3701.
[16] P. Hennebelle,et al. Turbulent molecular clouds , 2012, 1211.0637.
[17] J. Hough,et al. The Efficiency of Grain Alignment in Dense Interstellar Clouds: a Reassessment of Constraints from Near-Infrared Polarization , 2007, 0711.2536.
[18] Di Li,et al. THE MAGNETIC FIELD IN TAURUS PROBED BY INFRARED POLARIZATION , 2011, 1108.0410.
[19] G. Lagache,et al. Statistical properties of dust far-infrared emission , 2007, 0704.2175.
[20] B. Wandelt,et al. MAGNETIC FIELDS IN INTERSTELLAR CLOUDS FROM ZEEMAN OBSERVATIONS: INFERENCE OF TOTAL FIELD STRENGTHS BY BAYESIAN ANALYSIS , 2010 .
[21] A. Goodman,et al. Does near-infrared polarimetry reveal the magnetic field in cold dark clouds? , 1995 .
[22] G. Kowal,et al. Studies of Regular and Random Magnetic Fields in the ISM: Statistics of Polarization Vectors and the Chandrasekhar-Fermi Technique , 2008, 0801.0279.
[23] T. Murphy,et al. GASS: The Parkes Galactic All-Sky Survey. II. Stray-Radiation Correction and Second Data Release , 2010, 1007.0686.
[24] Joshua O. Gundersen,et al. LUPUS I OBSERVATIONS FROM THE 2010 FLIGHT OF THE BALLOON-BORNE LARGE APERTURE SUBMILLIMETER TELESCOPE FOR POLARIMETRY , 2013, 1307.5853.
[25] India,et al. Optical and submillimetre observations of Bok globules – tracing the magnetic field from low to high density , 2009, 0906.0248.
[26] P. Bastien,et al. GRAIN ALIGNMENT IN STARLESS CORES , 2014, 1411.1031.
[27] B. Draine,et al. Infrared extinction and polarization due to partially aligned spheroidal grains: Models for the dust toward the BN object , 1985 .
[28] N. Peretto,et al. TWO MASS DISTRIBUTIONS IN THE L 1641 MOLECULAR CLOUDS: THE HERSCHEL CONNECTION OF DENSE CORES AND FILAMENTS IN ORION A , 2013, 1309.2332.
[29] L. Hartmann,et al. EFFECTS OF MAGNETIC FIELD STRENGTH AND ORIENTATION ON MOLECULAR CLOUD FORMATION , 2008, 0812.3339.
[30] Zhi-Yun Li,et al. Magnetically Regulated Star Formation in Three Dimensions: The Case of the Taurus Molecular Cloud Complex , 2008, 0804.4201.
[31] C. A. Oxborrow,et al. Planck 2013 results. XIII. Galactic CO emission , 2013, 1303.5073.
[32] The Magnetic Field of Cloud 3 in L204 , 2014, 1407.3279.
[33] J. Peek,et al. MAGNETICALLY ALIGNED H i FIBERS AND THE ROLLING HOUGH TRANSFORM , 2013, 1312.1338.
[34] A. Goodman,et al. On the dispersion in direction of interstellar polarization , 1991 .
[35] S. Miyama,et al. An Origin of Filamentary Structure in Molecular Clouds , 1998 .
[36] C. B. Netterfield,et al. COMPARISON OF PRESTELLAR CORE ELONGATIONS AND LARGE-SCALE MOLECULAR CLOUD STRUCTURES IN THE LUPUS I REGION , 2014, 1405.0331.
[37] R. B. Barreiro,et al. Planck 2013 results. V. LFI calibration , 2013, 1303.5066.
[38] E. Mortsell. Calibrating Milky Way dust extinction using cosmological sources , 2012, 1210.2191.
[39] C. Horellou,et al. Magnetic fields and spiral arms in the galaxy M51 , 2010, 1001.5230.
[40] G. W. Pratt,et al. Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust , 2014, 1405.0871.
[41] B. M. Gaensler,et al. PROPERTIES OF INTERSTELLAR TURBULENCE FROM GRADIENTS OF LINEAR POLARIZATION MAPS , 2011, 1111.3544.
[42] T. Mouschovias,et al. Ambipolar Diffusion, Interstellar Dust, and the Formation of Cloud Cores and Protostars. I. Basic Physics and Formulation of the Problem , 1993 .
[43] The link between magnetic fields and filamentary clouds: bimodal cloud orientations in the Gould Belt , 2013, 1310.6261.
[44] R. Beck. Magnetism in the spiral galaxy NGC 6946: magnetic arms, depolarization rings, dynamo modes, and helical fields , 2007, 0705.4163.
[45] James M. Stone,et al. Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models , 2000, astro-ph/0008454.
[46] K. Gorski,et al. HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere , 2004, astro-ph/0409513.
[47] C. Brunt,et al. Trans-Alfvénic motions in the Taurus molecular cloud , 2011, 1110.0808.
[48] J. Fiege,et al. Polarized Submillimeter Emission from Filamentary Molecular Clouds , 2000, astro-ph/0005363.
[49] R. B. Barreiro,et al. Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps , 2014, 1411.2271.
[50] G. W. Pratt,et al. Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence , 2014, 1405.0872.
[51] Antonio Pereyra,et al. Polarimetry toward the Musca Dark Cloud. I. The Catalog , 2004 .
[52] Reconnection in a weakly stochastic field , 1998, astro-ph/9811037.
[53] R. Klessen,et al. From the warm magnetized atomic medium to molecular clouds , 2008, 0805.1366.
[54] C. B. Netterfield,et al. Planck early results. XIX. All-sky temperature and dust optical depth from Planck and IRAS. Constraints on the "dark gas" in our Galaxy , 2011, 1101.2029.
[55] J. Dickey,et al. Magnetically Dominated Strands of Cold Hydrogen in the Riegel-Crutcher Cloud , 2006, astro-ph/0608585.
[56] P. Hennebelle. On the origin of non-self-gravitating filaments in the ISM , 2013, 1306.5452.
[57] L. Hartmann,et al. Formation of Structure in Molecular Clouds: A Case Study , 2005, astro-ph/0507567.
[58] J. Dickey,et al. Infrared polarimetry and the galactic magnetic field. II: Improved models , 1992 .
[59] P. A. R. Ade,et al. Planck early results - XXIV. Dust in the diffuse interstellar medium and the galactic halo , 2011, 1101.2036.
[60] L. Spitzer,et al. Note on the collapse of magnetic interstellar clouds. , 1976 .
[61] J. Cardoso,et al. The local theory of the cosmic skeleton , 2008, 0811.1530.
[62] California Institute of Technology,et al. Dispersion of Magnetic Fields in Molecular Clouds , 2008 .
[63] California Institute of Technology,et al. DISPERSION OF MAGNETIC FIELDS IN MOLECULAR CLOUDS. III. , 2011 .
[64] E. Zweibel. Ambipolar Drift in a Turbulent Medium , 2001, astro-ph/0107462.
[65] University of Chicago,et al. Statistical Assessment of Shapes and Magnetic Field Orientations in Molecular Clouds through Polarization Observations , 2009, 0907.3730.
[66] The Millennium Arecibo 21 Centimeter Absorption-Line Survey. IV. Statistics of Magnetic Field, Column Density, and Turbulence , 2005, astro-ph/0501482.
[67] Alyssa A. Goodman,et al. Optical polarization maps of star-forming regions in Perseus, Taurus, and Ophiuchus , 1990 .
[68] A. Basu,et al. Magnetic fields in nearby normal galaxies: energy equipartition , 2013, 1305.2746.
[69] L. Blitz,et al. THE ORIGIN AND LIFETIME OF GIANT MOLECULAR CLOUD COMPLEXES , 1980 .
[70] Douglas P. Finkbeiner,et al. MEASURING REDDENING WITH SLOAN DIGITAL SKY SURVEY STELLAR SPECTRA AND RECALIBRATING SFD , 2010, 1012.4804.
[71] Jessie L. Dotson,et al. Tracing the Magnetic Field in Orion A , 2004 .
[72] H. Roussel,et al. From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey , 2010, 1005.2618.
[73] C. B. Netterfield,et al. AN IMPRINT OF MOLECULAR CLOUD MAGNETIZATION IN THE MORPHOLOGY OF THE DUST POLARIZED EMISSION , 2013, 1303.1830.
[74] G. W. Pratt,et al. Planck intermediate results. XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies , 2013, 1312.5446.
[75] J. Stil,et al. CHARACTERIZING MAGNETIZED TURBULENCE IN M51 , 2013, 1301.7508.
[76] F. Shu,et al. The gravitational collapse of a uniform spheroid. , 1965 .
[77] S. Poppi,et al. Galactic interstellar turbulence across the southern sky seen through spatial gradients of the polarization vector , 2014, 1404.6077.
[78] P. Koch,et al. EVOLUTION OF MAGNETIC FIELDS IN HIGH-MASS STAR FORMATION: LINKING FIELD GEOMETRY AND COLLAPSE FOR THE W51 e2/e8 CORES , 2009, 0905.1996.
[79] Magnetic fields in molecular clouds , 2012 .
[80] P. Hennebelle,et al. Thermal condensation in a turbulent atomic hydrogen flow , 2004 .
[81] C. A. Oxborrow,et al. Planck 2013 results - VIII. HFI photometric calibration and mapmaking , 2013, 1303.5069.
[82] G. W. Pratt,et al. Planck 2013 results. XI. All-sky model of thermal dust emission , 2013, 1312.1300.
[83] E. Parker,et al. Stochastic aspects of magnetic lines of force with application to cosmic-ray propagation. , 1969 .
[84] David O. Jones,et al. USING M DWARF SPECTRA TO MAP EXTINCTION IN THE LOCAL GALAXY , 2011, 1102.0280.
[85] Brenda C. Matthews,et al. THE LEGACY OF SCUPOL: 850 μm IMAGING POLARIMETRY FROM 1997 TO 2005 , 2009 .
[86] D. Hartmann,et al. The Milky Way in Molecular Clouds: A New Complete CO Survey , 2000, astro-ph/0009217.
[87] K. Chyży. Magnetic fields and gas in the cluster-influenced spiral galaxy NGC 4254. II. Structures of magnetic fields , 2007, 0712.4175.
[88] T. Jones. Infrared polarimetry and the interstellar magnetic field , 1989 .
[89] R. B. Barreiro,et al. Planck 2013 results. II. Low Frequency Instrument data processing , 2013, 1303.5063.
[90] Bonn,et al. Magnetic fields in barred galaxies - IV. NGC 1097 and NGC 1365 , 2005, astro-ph/0508485.
[91] C. A. Oxborrow,et al. Planck2013 results. VI. High Frequency Instrument data processing , 2013, Astronomy & Astrophysics.