THE MAGNETIZED ENVIRONMENT OF THE W3(H2O) PROTOSTARS
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H. Chen | D. Wilner | R. Rao | Sheng-Yuan Liu
[1] R. Klein,et al. SUB-ALFVÉNIC NON-IDEAL MAGNETOHYDRODYNAMIC TURBULENCE SIMULATIONS WITH AMBIPOLAR DIFFUSION. III. IMPLICATIONS FOR OBSERVATIONS AND TURBULENT ENHANCEMENT , 2011, 1109.3016.
[2] H. Chen,et al. DISKS AND OUTFLOWS IN THE MASSIVE PROTOBINARY SYSTEM W3(OH)TW , 2011, 1108.4899.
[3] G. Anglada,et al. A Magnetized Jet from a Massive Protostar , 2010, Science.
[4] N. Evans,et al. THE PROPERTIES OF MASSIVE, DENSE CLUMPS: MAPPING SURVEYS OF HCN AND CS , 2010, 1004.0398.
[5] J. Rathborne,et al. THE EARLY STAGES OF STAR FORMATION IN INFRARED DARK CLOUDS: CHARACTERIZING THE CORE DUST PROPERTIES , 2010, 1003.3193.
[6] Jessie L. Dotson,et al. 350 μm POLARIMETRY FROM THE CALTECH SUBMILLIMETER OBSERVATORY , 2010, 1001.2790.
[7] Qizhou Zhang,et al. Magnetic Fields in the Formation of Massive Stars , 2009, Science.
[8] 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.
[9] Brenda C. Matthews,et al. THE LEGACY OF SCUPOL: 850 μm IMAGING POLARIMETRY FROM 1997 TO 2005 , 2009 .
[10] P. Koch,et al. EVOLUTION OF MAGNETIC FIELDS IN HIGH MASS STAR FORMATION: SUBMILLIMETER ARRAY DUST POLARIZATION IMAGE OF THE ULTRACOMPACT H ii REGION G5.89−0.39 , 2008, 0812.3444.
[11] Daniel P. Marrone,et al. The submillimeter array polarimeter , 2008, Astronomical Telescopes + Instrumentation.
[12] E. Ostriker,et al. Theory of Star Formation , 2007, 0707.3514.
[13] A. Lazarian,et al. Tracing Magnetic Fields with Aligned Grains , 2007, 0707.0858.
[14] John E. Vaillancourt,et al. Placing Confidence Limits on Polarization Measurements , 2006, astro-ph/0603110.
[15] K. Menten,et al. Water Maser Motions in W3(OH) and a Determination of Its Distance , 2005, astro-ph/0512226.
[16] J. M. Moran,et al. Interferometric Measurements of Variable 340 GHz Linear Polarization in Sagittarius A* , 2005, astro-ph/0511653.
[17] W. Welch,et al. A High-Mass Protobinary System in the Hot Core W3(H2O) , 2005, astro-ph/0511294.
[18] Zhi-Yun Li,et al. Does Magnetic Levitation or Suspension Define the Masses of Forming Stars? , 2003, astro-ph/0311426.
[19] J. Girart,et al. Interferometric Mapping of Magnetic Fields in Star-forming Regions. III. Dust and CO Polarization in DR 21(OH) , 2003, astro-ph/0308051.
[20] Jingwen Wu,et al. Indications of Inflow Motions in Regions Forming Massive Stars , 2003, astro-ph/0306543.
[21] Magnetic Fields in Shocked Regions: Very Large Array Observations of H2O Masers , 2002 .
[22] B. Matthews,et al. Magnetic Fields in Star-forming Molecular Clouds. II. The Depolarization Effect in the OMC-3 Filament of Orion A , 2001, astro-ph/0106394.
[23] James M. Stone,et al. Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models , 2000, astro-ph/0008454.
[24] W. Holland,et al. First Observations of the Magnetic Field Geometry in Prestellar Cores , 2000, astro-ph/0006069.
[25] Jessie L. Dotson,et al. Far-Infrared Polarimetry of Galactic Clouds from the Kuiper Airborne Observatory , 2000 .
[26] B. Matthews,et al. Magnetic Fields in Star-forming Molecular Clouds. I. The First Polarimetry of OMC-3 in Orion A , 1999, astro-ph/9911148.
[27] K. Menten,et al. Hot Gas and Dust in a Protostellar Cluster near W3(OH) , 1999, astro-ph/9901261.
[28] E. Ostriker,et al. Low-Mass Star Formation: Theory , 1999 .
[29] Richard M. Crutcher,et al. Magnetic Fields in Molecular Clouds: Observations Confront Theory , 1998 .
[30] M. Wright,et al. High-Resolution Millimeter-Wave Mapping of Linearly Polarized Dust Emission: Magnetic Field Structure in Orion , 1998, astro-ph/9805288.
[31] K. Menten,et al. The Synchrotron Jet from the H2O Maser Source in W3(OH) , 1999 .
[32] Philip C. Myers,et al. On the Efficiency of Grain Alignment in Dark Clouds , 1997, astro-ph/9706163.
[33] G. Garay,et al. The Nature of the Radio Sources within the Cepheus A Star-forming Region , 1996 .
[34] K. Menten,et al. Synchrotron Emission from the H 2O Maser Source in W3(OH) , 1995 .
[35] W. Welch,et al. THE S140 CORE : APERTURE SYNTHESIS HCO+ AND SO OBSERVATIONS , 1994 .
[36] K. Miyake,et al. Effects of Particle Size Distribution on Opacity Curves of Protoplanetary Disks around T Tauri Stars , 1993 .
[37] B. Reipurth,et al. HH 80-81: A Highly collimated Herbig-Haro complex powered by a massive young star , 1993 .
[38] K. Johnston,et al. Ammonia in the W3(OH) Region , 1993 .
[39] The proper motions of the H 2 O masers near W3(OH). , 1993 .
[40] A. Goodman,et al. On the dispersion in direction of interstellar polarization , 1991 .
[41] F. Adams,et al. Star Formation in Molecular Clouds: Observation and Theory , 1987 .
[42] J. Turner,et al. Discovery of a young stellar object near the water masers in W3 (OH). , 1984 .
[43] Enrico Fermi,et al. Magnetic fields in spiral arms , 1953 .