JCMT BISTRO Survey: Magnetic Fields within the Hub-filament Structure in IC 5146
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E. Pascale | A. Scaife | P. Koch | A. Whitworth | N. Peretto | G. Fuller | H. Chen | T. Onaka | M. Tamura | Sang-Sung Lee | D. Byun | D. Johnstone | P. Bastien | Jongsoo Kim | G. Savini | J. Francesco | B. Matthews | Di Li | P. Friberg | M. Seta | J. Kwon | T. Nagata | Tsuyoshi Inoue | W. Chen | K. Kawabata | S. Eyres | S. Falle | M. Griffin | W. Holland | J. Greaves | G. Moriarty-Schieven | T. Hasegawa | D. Ward-Thompson | J. Hatchell | A. Chrysostomou | J. Fiege | R. Friesen | S. Graves | M. Houde | J. Kirk | J. Richer | P. Andr'e | K. Lacaille | C. Dowell | A. Kataoka | R. Rao | M. Rawlings | H. Parsons | Jia‐Wei Wang | L. Qian | K. Qiu | T. Ching | Jinghua Yuan | A. Rigby | Jianjun Zhou | Da-lei Li | G. Park | Miju Kang | Il-Gyo Jeong | H. Nakanishi | Jeong-Eun Lee | Kee-Tae Kim | Hongchi Wang | Tie Liu | Ji-hyun Kang | S. Inutsuka | F. Kemper | Minho Choi | Sung-ju Kang | Jungyeon Cho | H. Yoo | D. Berry | T. Pyo | F. Nakamura | S. Loo | V. Konyves | D. Arzoumanian | Guoyin Zhang | Junhao Liu | Y. Doi | J. Robitaille | Chuan-Peng Zhang | Hua-b. Li | Sheng-Yuan Liu | S. Lai | A. Soam | C. Lee | Ya-Wen Tang | Gwanjeong Kim | S. Mairs | Shinyoung Kim | K. Pattle | W. Kwon | E. Chung | A. Pon | H. Duan | S. Hayashi | M. Matsumura | Yapeng Zhang | S. Sadavoy | K. Tomisaka | Y. Tsukamoto | Hsi-Wei Yen | N. Ohashi | K. Iwasaki | Yusuke Aso | Chin-Fei Lee | H. Shinnaga | L. Fanciullo | M. C. Chen | E. Drabek-Maunder | T. Gledhill | Mi-Ryang Kim | R. Furuya | S. Coud'e | C. Eswaraiah | K. Kim | A. Lyo | B. Retter | I. Han | Hyeseung Lee | Thiem C. Hoang | Hyeong-Sik Yun | T. Zenko | Masato I. N. Kobayashi | E. Franzmann | Hong-Li Liu | Q. Gu | Yoshihiro Kanamori | H. Saito | J. Hwang | Yong-Hee Lee | Zhu | T. Inoue | S. Lai | Hongli Liu | Chuan-peng Zhang | W. Chen | H. Yun | Ya-wen Tang | Geumsook Park
[1] K. Menten,et al. Probing the initial conditions of high-mass star formation , 2007, Astronomy & Astrophysics.
[2] L. Loinard,et al. Distances and Kinematics of Gould Belt Star-forming Regions with Gaia DR2 Results , 2018, The Astrophysical Journal.
[3] Per Friberg,et al. Characterizing and reducing the POL-2 instrumental polarization , 2018, Astronomical Telescopes + Instrumentation.
[4] Tetsuo Hasegawa,et al. First Observations of the Magnetic Field inside the Pillars of Creation: Results from the BISTRO Survey , 2018, The Astrophysical Journal.
[5] Lei Zhu,et al. Magnetic Fields toward Ophiuchus-B Derived from SCUBA-2 Polarization Measurements , 2018, The Astrophysical Journal.
[6] T. A. Lister,et al. Gaia Data Release 2. Summary of the contents and survey properties , 2018, 1804.09365.
[7] Lei Zhu,et al. A First Look at BISTRO Observations of the ρ Oph-A core , 2018, 1804.09313.
[8] L. V. Tóth,et al. A Holistic Perspective on the Dynamics of G035.39-00.33: The Interplay between Gas and Magnetic Fields , 2018, The Astrophysical Journal.
[9] P. Koch,et al. Polarization Properties and Magnetic Field Structures in the High-mass Star-forming Region W51 Observed with ALMA , 2018, 1801.08264.
[10] E. Vázquez-Semadeni,et al. The magnetic field structure in molecular cloud filaments , 2018, Monthly Notices of the Royal Astronomical Society.
[11] P. Koch,et al. MAGNETIC FIELDS AND MASSIVE STAR FORMATION , 2014, Proceedings of the International Astronomical Union.
[12] A. Zavagno,et al. High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion in G22 , 2017, 1711.08951.
[13] Multiwavelength stellar polarimetry of the filamentary cloud IC5146. I. Dust properties , 2017, 1710.03899.
[14] P. Koch,et al. The JCMT BISTRO Survey: The Magnetic Field Strength in the Orion A Filament , 2017, 1707.05269.
[15] A. Goodman,et al. Unveiling the Role of the Magnetic Field at the Smallest Scales of Star Formation , 2017, 1706.03806.
[16] P. Koch,et al. Magnetized Converging Flows toward the Hot Core in the Intermediate/High-mass Star-forming Region NGC 6334 V , 2017, 1706.03534.
[17] Saeko S. Hayashi,et al. First Results from BISTRO: A SCUBA-2 Polarimeter Survey of the Gould Belt , 2017, 1704.08552.
[18] Qizhou Zhang,et al. A Massive Prestellar Clump Hosting No High-mass Cores , 2017, 1704.08264.
[19] A. Lazarian,et al. Alignment of Irregular Grains by Mechanical Torques , 2017, 1704.02256.
[20] Silvia De Francesco,et al. The JCMT Gould Belt Survey: A First Look at IC 5146 , 2017, 1701.04898.
[21] Qizhou Zhang,et al. MAGNETICALLY DOMINATED PARALLEL INTERSTELLAR FILAMENTS IN THE INFRARED DARK CLOUD G14.225-0.506 , 2016, 1609.08052.
[22] Giorgio Savini,et al. POL-2: a polarimeter for the James-Clerk-Maxwell telescope , 2016, Astronomical Telescopes + Instrumentation.
[23] R. Gehrz,et al. SOFIA MID-INFRARED IMAGING AND CSO SUBMILLIMETER POLARIMETRY OBSERVATIONS OF G034.43+00.24 MM1 , 2016 .
[24] John Salvatier,et al. Probabilistic programming in Python using PyMC3 , 2016, PeerJ Comput. Sci..
[25] A. Whitworth,et al. Perturbation growth in accreting filaments , 2016, 1602.07651.
[26] Qizhou Zhang,et al. HELICAL MAGNETIC FIELDS IN THE NGC 1333 IRAS 4A PROTOSTELLAR OUTFLOWS , 2016, 1601.05229.
[27] D. Johnstone,et al. The JCMT Gould Belt Survey: the effect of molecular contamination in SCUBA-2 observations of Orion A , 2016, 1601.01989.
[28] G. W. Pratt,et al. Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds , 2015, 1502.04123.
[29] J. Hough,et al. WIDE-FIELD INFRARED POLARIMETRY OF THE ρ OPHIUCHI CLOUD CORE , 2015 .
[30] J. Pineda,et al. The JCMT Gould Belt Survey: a quantitative comparison between SCUBA-2 data reduction methods , 2015, 1509.06385.
[31] John E. Vaillancourt,et al. Interstellar Dust Grain Alignment , 2015 .
[32] D. Johnstone,et al. YOUNG STELLAR OBJECTS IN THE GOULD BELT , 2015, 1508.03199.
[33] S. Inutsuka,et al. The Formation and Destruction of Molecular Clouds and Galactic Star Formation , 2015, Proceedings of the International Astronomical Union.
[34] Ludmilla Kolokolova,et al. Polarimetry of Stars and Planetary Systems , 2015 .
[35] H. Liu,et al. ALMA resolves the spiraling accretion flow in the luminous OB cluster forming region G33.92+0.11 , 2015, 1505.04255.
[36] P. K. Leung,et al. Self-similar fragmentation regulated by magnetic fields in a region forming massive stars , 2015, Nature.
[37] S. Walch,et al. The impact of turbulence and magnetic field orientation on star-forming filaments , 2015, 1503.01659.
[38] S. Plaszczynski,et al. Polarization measurement analysis - I. Impact of the full covariance matrix on polarization fraction and angle measurements , 2014, 1406.6536.
[39] P. Koch,et al. THE IMPORTANCE OF THE MAGNETIC FIELD FROM AN SMA–CSO-COMBINED SAMPLE OF STAR-FORMING REGIONS , 2014, 1411.3830.
[40] L. Montier,et al. Polarization measurements analysis II. Best estimators of polarization fraction and angle , 2014, 1407.0178.
[41] Qizhou Zhang,et al. CORE AND FILAMENT FORMATION IN MAGNETIZED, SELF-GRAVITATING ISOTHERMAL LAYERS , 2014, 1405.1013.
[42] T. Henning,et al. The link between magnetic fields and filamentary clouds: bimodal cloud orientations in the Gould Belt , 2013, 1310.6261.
[43] J. Francesco,et al. Abundant Cyanopolyynes as a Probe of Infall in the Serpens South Cluster-Forming Region , 2013, 1309.1763.
[44] E. Vázquez-Semadeni,et al. FILAMENTS IN SIMULATIONS OF MOLECULAR CLOUD FORMATION , 2013, 1308.6298.
[45] Prasanth H. Nair,et al. Astropy: A community Python package for astronomy , 2013, 1307.6212.
[46] G. Wilson,et al. FILAMENTARY ACCRETION FLOWS IN THE EMBEDDED SERPENS SOUTH PROTOCLUSTER , 2013, 1301.6792.
[47] Per Friberg,et al. Scuba-2: On-sky calibration using submillimetre standard sources , 2013, 1301.3773.
[48] Douglas Scott,et al. Scuba-2: Iterative map-making with the sub-millimetre user reduction facility , 2013, 1301.3652.
[49] P. A. R. Ade,et al. SCUBA-2: the 10 000 pixel bolometer camera on the James Clerk Maxwell Telescope , 2013, 1301.3650.
[50] Astrophysics,et al. UNVEILING A NETWORK OF PARALLEL FILAMENTS IN THE INFRARED DARK CLOUD G14.225−0.506 , 2012, The Astrophysical Journal.
[51] D. Johnstone,et al. ASPECT RATIO DEPENDENCE OF THE FREE-FALL TIME FOR NON-SPHERICAL SYMMETRIES , 2012, 1207.3078.
[52] Fragmentation and OB Star Formation in High-Mass Molecular Hub-Filament Systems , 2012, 1206.1907.
[53] D. Johnstone,et al. Molecular line contamination in the SCUBA-2 450 and 850 μm continuum data , 2012, 1204.6180.
[54] O. Miettinen. A molecular line study of the filamentary infrared dark cloud G304.74+01.32 , 2012, 1202.3051.
[55] Jason L. Quinn,et al. Bayesian analysis of polarization measurements , 2012, 1202.0299.
[56] P. Bastien,et al. GRAIN ALIGNMENT IN STARLESS CORES , 2014, 1411.1031.
[57] Adam Ginsburg,et al. PySpecKit: Python Spectroscopic Toolkit , 2011 .
[58] D. Johnstone,et al. MODES OF STAR FORMATION IN FINITE MOLECULAR CLOUDS , 2011, 1108.1395.
[59] M. Tamura,et al. NEAR-INFRARED-IMAGING POLARIMETRY TOWARD SERPENS SOUTH: REVEALING THE IMPORTANCE OF THE MAGNETIC FIELD , 2011, 1104.2977.
[60] N. Peretto,et al. Astronomy Astrophysics Letter to the Editor Characterizing interstellar filaments with Herschel in IC 5146 ⋆,⋆⋆ , 2022 .
[61] Gaël Varoquaux,et al. The NumPy Array: A Structure for Efficient Numerical Computation , 2011, Computing in Science & Engineering.
[62] Peng Wang,et al. LOWERING THE CHARACTERISTIC MASS OF CLUSTER STARS BY MAGNETIC FIELDS AND OUTFLOW FEEDBACK , 2010, 1008.0409.
[63] 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.
[64] D. Marrone,et al. IRAS 16293: A “MAGNETIC” TALE OF TWO CORES , 2009, 0910.5269.
[65] T. Jenness,et al. HARP/ACSIS: a submillimetre spectral imaging system on the James Clerk Maxwell Telescope , 2009, 0907.3610.
[66] P. Myers. FILAMENTARY STRUCTURE OF STAR-FORMING COMPLEXES , 2009, 0906.2005.
[67] 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.
[68] A. Lazarian,et al. RADIATIVE TORQUES ALIGNMENT IN THE PRESENCE OF PINWHEEL TORQUES , 2008, 0801.0266.
[69] J. Dotson,et al. DISPERSION OF MAGNETIC FIELDS IN MOLECULAR CLOUDS. I , 2009 .
[70] Jessie L. Dotson,et al. DISPERSION OF MAGNETIC FIELDS IN MOLECULAR CLOUDS. II. , 2008, 0909.5227.
[71] L. Allen,et al. The Spitzer Survey of Interstellar Clouds in the Gould Belt. I. IC 5146 Observed With IRAC and MIPS , 2008 .
[72] Zhi-Yun Li,et al. Magnetically Regulated Star Formation in Three Dimensions: The Case of the Taurus Molecular Cloud Complex , 2008, 0804.4201.
[73] Daniel J. Price,et al. The effect of magnetic fields on star cluster formation , 2008, 0801.3293.
[74] J. Hough,et al. The Efficiency of Grain Alignment in Dense Interstellar Clouds: a Reassessment of Constraints from Near-Infrared Polarization , 2007, 0711.2536.
[75] A. Lazarian,et al. Subsonic Mechanical Alignment of Irregular Grains , 2007, 0707.3805.
[76] A. Lazarian,et al. Radiative torques: analytical model and basic properties , 2007, 0707.0886.
[77] Ramprasad Rao,et al. Magnetic Fields in the Formation of Sun-Like Stars , 2006, Science.
[78] John E. Vaillancourt,et al. Placing Confidence Limits on Polarization Measurements , 2006, astro-ph/0603110.
[79] C. Aspin,et al. Astronomical Polarimetry: Current Status and Future Directions , 2005 .
[80] W. D. Watson,et al. Line Polarization of Molecular Lines at Radio Frequencies: The Case of DR 21(OH) , 2005, astro-ph/0504258.
[81] K. Rice,et al. Protostars and Planets V , 2005 .
[82] M. Juvela,et al. Theoretical Models of Polarized Dust Emission from Protostellar Cores , 2001, astro-ph/0104231.
[83] M. Norman,et al. Magnetic Field Diagnostics Based on Far-Infrared Polarimetry: Tests Using Numerical Simulations , 2001, astro-ph/0103286.
[84] J. Weingartner,et al. Dust Grain-Size Distributions and Extinction in the Milky Way, Large Magellanic Cloud, and Small Magellanic Cloud , 2001 .
[85] James M. Stone,et al. Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models , 2000, astro-ph/0008454.
[86] A. Boss,et al. Protostars and Planets VI , 2000 .
[87] J. Alves,et al. Infrared Extinction and the Structure of the IC 5146 Dark Cloud , 1999 .
[88] S. Miyama,et al. An Origin of Filamentary Structure in Molecular Clouds , 1998 .
[89] Philip C. Myers,et al. On the Efficiency of Grain Alignment in Dark Clouds , 1997, astro-ph/9706163.
[90] R. Crutcher. Magnetic fields in molecular clouds , 2007 .
[91] F. Bertoldi,et al. Pressure-confined clumps in magnetized molecular clouds , 1992 .
[92] T. Jones. Infrared polarimetry and the interstellar magnetic field , 1989 .
[93] M. Tamura,et al. Infrared polarimetry of dark clouds – I. Magnetic field structure in Heiles Cloud 2 , 1987 .
[94] T. Mouschovias,et al. The effect of ambipolar diffusion on magnetic braking of molecular cloud cores: an exact, time-dependent solution , 1986 .
[95] W. D. Watson,et al. Linear polarization of molecular lines at radio frequencies , 1984 .
[96] N. Kylafis,et al. Linear polarization of radio frequency lines in molecular clouds and circumstellar envelopes , 1982 .
[97] N. Kylafis,et al. On mapping the magnetic field direction in molecular clouds by polarization measurements , 1981 .
[98] J. Wardle,et al. The linear polarization of quasi-stellar radio sources at 3.71 and 11.1 centimeters. , 1974 .
[99] Enrico Fermi,et al. Magnetic fields in spiral arms , 1953 .
[100] S. Rice. Mathematical analysis of random noise , 1944 .