Magnetic Fields in the Multiphase Interstellar Medium

We discuss the interstellar magnetic field and its measurement in the different phases of the interstellar medium. The measurement techniques include Faraday rotation, Zeeman splitting, linear polarization from aligned dust grains, and the Chandrasekhar-Fermi method. The phases include the classical ones: molecular clouds, the Cold and Warm Neutral Media, the Warm and Hot Ionized Media. We also include a less well-known phase, the Warm Partially Ionized Medium, which can be surprisingly prominent in Faraday rotation.

[1]  R. Pudritz,et al.  The formation of star clusters – II. 3D simulations of magnetohydrodynamic turbulence in molecular clouds , 2005, astro-ph/0508562.

[2]  Magnetic Fields in Shocked Regions: Very Large Array Observations of H2O Masers , 2002 .

[3]  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.

[4]  松本 仁,et al.  Cosmic Magnetic Fields : from Planets, to Stars and Galaxies , 2009 .

[5]  J. Stil,et al.  A ROTATION MEASURE IMAGE OF THE SKY , 2009 .

[6]  A. Tielens TETONS 4: GALACTIC STRUCTURE, STARS, AND THE INTERSTELLAR MEDIUM , 2001 .

[7]  D. Burrows,et al.  X-Ray Morphology, Kinematics, and Geometry of the Eridanus Soft X-Ray Enhancement , 1994 .

[8]  C. Norman,et al.  Density Structure of the Interstellar Medium and the Star Formation Rate in Galactic Disks , 2007, astro-ph/0701595.

[9]  California Institute of Technology,et al.  DISPERSION OF MAGNETIC FIELDS IN MOLECULAR CLOUDS. III. , 2011 .

[10]  W. B. Burton,et al.  The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI - Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections , 2005, astro-ph/0504140.

[11]  P. Padoan,et al.  THE STAR FORMATION RATE OF SUPERSONIC MAGNETOHYDRODYNAMIC TURBULENCE , 2009, 0907.0248.

[12]  U. Colorado,et al.  The Structure of the Local Interstellar Medium. III. Temperature and Turbulence , 2004, astro-ph/0406464.

[13]  G. Novak,et al.  DISPERSION OF OBSERVED POSITION ANGLES OF SUBMILLIMETER POLARIZATION IN MOLECULAR CLOUDS , 2007, 0707.2818.

[14]  Simon Prunet,et al.  Statistical Properties of Galactic Starlight Polarization , 2001, astro-ph/0105023.

[15]  M. Maclow Turbulence in the Interstellar Medium , 2004 .

[16]  R. Güsten,et al.  Strong magnetic fields in interstellar H2O maser clumps , 1989 .

[17]  E. Pellegrini,et al.  A Magnetically Supported Photodissociation Region in M17 , 2006, astro-ph/0611808.

[18]  Jeffrey L. Linsky,et al.  The Structure of the Local Interstellar Medium. IV. Dynamics, Morphology, Physical Properties, and Implications of Cloud-Cloud Interactions , 2007, 0709.4480.

[19]  Dan McCammon,et al.  ROSAT Survey Diffuse X-Ray Background Maps. II. , 1997 .

[20]  R. Beck,et al.  Cosmic magnetic fields , 2005 .

[21]  California Institute of Technology,et al.  Dispersion of Magnetic Fields in Molecular Clouds , 2008 .

[22]  M. Wolleben,et al.  A New Model for the Loop I (North Polar Spur) Region , 2007, 0704.0276.

[23]  J. Ostriker,et al.  A theory of the interstellar medium - Three components regulated by supernova explosions in an inhomogeneous substrate , 1977 .

[24]  K. Tassis,et al.  Testing Molecular-Cloud Fragmentation Theories: Self-Consistent Analysis of OH Zeeman Observations , 2009, 0909.2031.

[25]  C. Brogan,et al.  VLA H I and OH Zeeman Observations toward M17 , 2001 .

[26]  R. Beck Galactic and Extragalactic Magnetic Fields , 2000, astro-ph/0012402.

[27]  E. Fitzpatrick,et al.  Composition of Interstellar Clouds in the Disk and Halo. IV. HD 215733 , 1993 .

[28]  S. Basu Magnetic Fields and the Triaxiality of Molecular Cloud Cores , 2000, astro-ph/0008243.

[29]  Edward B. Jenkins,et al.  The Distribution of Thermal Pressures in the Interstellar Medium , 2001 .

[30]  The Neutral Atomic Phases of the ISM in the Galaxy , 2002, astro-ph/0207098.

[31]  Revised equipartition and minimum energy formula for magnetic field strength estimates from radio synchrotron observations , 2005, astro-ph/0507367.

[32]  C. Heiles The Local Direction and Curvature of the Galactic Magnetic Field Derived from Starlight Polarization , 1996 .

[33]  Jeffrey W. Percival,et al.  The Wisconsin Hα Mapper Northern Sky Survey , 2001 .

[34]  P. Hennebelle,et al.  On the structure of the turbulent interstellar clouds . Influence of the equation of state on the dynamics of 3D compressible flows , 2009, 0911.0748.

[35]  A. Tielens,et al.  Neutral Atomic Phases of the Interstellar Medium in the Galaxy , 2003 .

[36]  K. Menten,et al.  Interstellar Hydroxyl Masers in the Galaxy. II. Zeeman Pairs and the Galactic Magnetic Field , 2003, astro-ph/0307156.

[37]  I. Pérez,et al.  FORMATION AND EVOLUTION OF GALAXY DISKS , 2008 .

[38]  Richard M. Crutcher,et al.  TESTING MAGNETIC STAR FORMATION THEORY , 2008, 0807.2862.

[39]  C. Heiles,et al.  Magnetic fields in diffuse HI and molecular clouds , 2005, astro-ph/0501550.

[40]  Richard M. Crutcher,et al.  CN Zeeman measurements in star formation regions , 2008 .

[41]  L. M. Haffner The Wisconsin H-Alpha Mapper Northern Sky Survey , 2000, astro-ph/0010097.

[42]  J. Dickey,et al.  Milky Way Kinematics: Measurements at the Subcentral Point of the Fourth Quadrant , 2007, 0708.0870.