| Magnetic Fields in the Early Universe |
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1 | (8) |
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1 | (1) |
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2 Magnetic Fields from the Ultra-Early Universe? |
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2 | (2) |
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3 Protogalactic Batteries |
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4 | (1) |
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4 Magnetic Fields from the First Stars |
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5 | (1) |
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6 | (1) |
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7 | (1) |
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7 | (2) |
| Magnetic Fields in Galaxy Systems, Clusters and Beyond |
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9 | (32) |
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1 Introduction and Background |
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9 | (1) |
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2 Stellar Sources of Extragalactic Magnetic Fields |
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10 | (4) |
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3 Early Plasma-driven Seeding Scenarios |
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14 | (1) |
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4 The Galactic Large-scale α Ω Dynamo Theory |
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14 | (1) |
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5 Proxy Measurements for Cosmologically Early, Star-ejected Magnetic Fields |
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15 | (1) |
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6 Post-amplification of Initially Weak Intergalactic Seed Fields of All Kinds |
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16 | (1) |
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7 Massive Black Hole Seeding of Intergalactic Magnetic Fields |
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17 | (4) |
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8 Gravitational Collapse and Black Hole Electromagnetic Energy Generators |
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21 | (3) |
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9 Radio Galaxies as 'Calorimeters' of BH-injected Magnetic Fields and CR's |
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24 | (2) |
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10 Magnetic Fields in Clusters of Galaxies |
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26 | (6) |
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11 Probes of Magnetic Fields at Larger Redshifts, Beyond Galaxies and Clusters |
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32 | (5) |
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37 | (1) |
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37 | (4) |
| Magnetic Fields in Galaxies |
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41 | (28) |
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41 | (1) |
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2 Observing Extragalactic Magnetic Fields |
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41 | (2) |
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3 Measuring Magnetic Field Strengths |
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43 | (2) |
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4 Magnetic Fields and Gas Clouds |
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45 | (2) |
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5 Magnetic Field Structure |
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47 | (6) |
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53 | (2) |
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7 Magnetic Fields in Flocculent and Irregular Galaxies |
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55 | (1) |
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8 Magnetic Fields in Barred Galaxies |
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56 | (3) |
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59 | (2) |
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61 | (2) |
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11 Spiral Galaxies with Jets |
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63 | (1) |
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64 | (1) |
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65 | (4) |
| The Origin of Galactic Magnetic Fields |
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69 | (20) |
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69 | (1) |
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2 The Alpha-Omega Disc Dynamo |
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70 | (5) |
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3 Evolution of a Primordial Magnetic Field |
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75 | (7) |
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4 The Protogalactic Dynamo |
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82 | (5) |
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87 | (1) |
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88 | (1) |
| Magnetic Fields in the Milky Way, Derived from Radio Continuum Observations and Faraday Rotation Studies |
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89 | (24) |
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89 | (1) |
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2 Observational Rationale |
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90 | (3) |
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3 The Earliest Observations |
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93 | (1) |
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4 Radio Continuum Surveys of the Milky Way |
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94 | (8) |
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5 Surveys of Rotation Measure of Extragalactic Radio Sources (EGRS) |
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102 | (2) |
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6 Pulsars as Probes of the Magnetic Fields of the Galaxy |
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104 | (1) |
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7 The Magnetic Fields of the Milky Way |
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105 | (3) |
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108 | (5) |
| Mesoscale Magnetic Structures in Spiral Galaxies |
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113 | (24) |
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113 | (1) |
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2 Observational Evidence for Magnetic Reversals |
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114 | (3) |
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117 | (6) |
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123 | (2) |
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125 | (8) |
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133 | (1) |
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133 | (4) |
| Magnetic Fields in Diffuse H1 and Molecular Clouds |
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Carl Heiles, Richard Crutcher |
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137 | (46) |
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137 | (2) |
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2 Measuring the Magnetic Field in Diffuse H i and Molecular Clouds |
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139 | (7) |
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3 Observed vs. Intrinsic Probability Density Functions |
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146 | (7) |
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4 B|| from H1 Absorption Lines |
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153 | (4) |
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5 B|| from H1 Emission Lines |
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157 | (6) |
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6 Importance of Magnetic Fields in Molecular Clouds |
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163 | (1) |
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7 Molecular Cloud Observational Results |
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164 | (6) |
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8 Model Predictions and Observational Tests |
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170 | (6) |
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9 Magnetic Field Observations, Present and Future |
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176 | (3) |
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179 | (4) |
| Stellar Magnetic Fields |
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Leon Mestel, John D. Landstreet |
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183 | (36) |
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183 | (5) |
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2 Magnetism and Star Formation |
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188 | (3) |
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3 Pre-main Sequence Stars: Observation and Theory |
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191 | (2) |
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4 The Main-sequence: Late-type Stars |
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193 | (7) |
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5 The Main Sequence: Early-type Stars |
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200 | (7) |
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6 The Early-type Magnetic Stars: Basic Theoretical Questions |
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207 | (4) |
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211 | (1) |
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212 | (1) |
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213 | (6) |
| Importance of Magnetic Helicity in Dynamos |
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219 | (36) |
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219 | (2) |
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2 Dynamos in a Periodic Box |
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221 | (2) |
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3 Magnetic Helicity Evolution |
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223 | (5) |
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4 What Do Stars and Galaxies Do Differently'? |
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228 | (7) |
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5 Connection with the a Effect |
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235 | (9) |
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6 What about η Quenching'? |
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244 | (6) |
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250 | (1) |
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251 | (4) |
| Numerical Magnetohydrodynamics in Astrophysics |
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255 | |
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255 | (1) |
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2 The Classical MHD Model in Computer Simulation |
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256 | (7) |
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3 Progress in Understanding Fundamental MHD Processes |
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263 | (7) |
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4 Special Relativistic MHD (SRMHD) Limits of the Classical MHD |
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270 | (3) |
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5 Relativistic MHD for Rotating Black Holes (GRMHD) |
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273 | (4) |
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277 | (1) |
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278 | |
