Preface to the second edition |
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xiii | |
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Dust in the Galaxy: Our view from within |
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1 | (37) |
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1 | (1) |
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Historical perspective: Discovery and assimilation |
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2 | (6) |
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The distribution of dust and gas |
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8 | (7) |
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8 | (2) |
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10 | (2) |
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12 | (1) |
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Diffuse galactic background radiation |
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13 | (2) |
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Interstellar environments and physical processes |
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15 | (9) |
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15 | (1) |
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The physical state of the interstellar medium |
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15 | (3) |
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18 | (3) |
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21 | (1) |
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The interstellar environment of the Solar System |
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22 | (2) |
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The significance of dust in modern astrophysics |
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24 | (4) |
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From Cinderella to the search for origins |
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24 | (1) |
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Interstellar processes and chemistry |
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24 | (2) |
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Stars, nebulae and galaxies |
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26 | (1) |
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27 | (1) |
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A brief history of models for interstellar dust |
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28 | (10) |
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Dirty ices, metals and Platt particles |
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29 | (1) |
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30 | (3) |
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Unmantled refractory and core/mantle models |
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33 | (2) |
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35 | (1) |
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35 | (1) |
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36 | (2) |
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Abundances and depletions |
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38 | (28) |
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The origins of the condensible elements |
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39 | (6) |
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The cosmic cycle: an overview |
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39 | (2) |
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41 | (1) |
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41 | (3) |
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Enrichment of the interstellar medium |
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44 | (1) |
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The Solar System abundances |
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45 | (5) |
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Significance and methodology |
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45 | (1) |
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46 | (4) |
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Abundance trends in the Galaxy |
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50 | (4) |
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50 | (1) |
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51 | (2) |
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Solar abundances in space and time |
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53 | (1) |
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54 | (7) |
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54 | (2) |
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Average depletions in diffuse clouds |
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56 | (3) |
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Dependence on environment |
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59 | (1) |
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60 | (1) |
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Implications for grain models |
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61 | (5) |
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64 | (1) |
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64 | (2) |
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Extinction and scattering |
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66 | (46) |
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67 | (5) |
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Extinction by spherical particles |
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67 | (2) |
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Small-particle approximations |
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69 | (1) |
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Albedo, scattering function and asymmetry parameter |
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70 | (1) |
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71 | (1) |
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72 | (3) |
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The average extinction curve and albedo |
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75 | (9) |
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The average extinction curve |
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75 | (2) |
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Scattering characteristics |
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77 | (3) |
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Long-wavelength extinction and evaluation of Rv |
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80 | (2) |
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82 | (1) |
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Dust density and dust-to-gas ratio |
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83 | (1) |
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84 | (7) |
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84 | (4) |
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88 | (3) |
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91 | (1) |
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The 2175 Å absorption feature |
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91 | (11) |
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92 | (5) |
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Implications for the identity of the carrier |
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97 | (5) |
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102 | (4) |
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Modelling the interstellar extinction curve |
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106 | (6) |
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109 | (1) |
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109 | (3) |
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Polarization and grain alignment |
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112 | (42) |
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Extinction by anisotropic particles |
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113 | (2) |
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Polarimetry and the structure of the galactic magnetic field |
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115 | (10) |
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115 | (2) |
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117 | (3) |
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120 | (2) |
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122 | (1) |
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Dense clouds and the skin-depth effect |
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123 | (2) |
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The spectral dependence of polarization |
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125 | (13) |
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125 | (2) |
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Power-law behaviour in the infrared |
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127 | (1) |
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Polarization and extinction |
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128 | (4) |
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132 | (5) |
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137 | (1) |
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Polarization and grain models |
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138 | (3) |
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141 | (13) |
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Grain spin and rotational dissipation |
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142 | (3) |
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Paramagnetic relaxation: the DG mechanism |
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145 | (2) |
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Superparamagnetic alignment |
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147 | (1) |
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148 | (1) |
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149 | (1) |
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150 | (1) |
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Alignment in dense clouds |
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151 | (1) |
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152 | (1) |
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152 | (2) |
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Infrared absorption features |
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154 | (41) |
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Basics of infrared spectroscopy |
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155 | (7) |
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Vibrational modes in solids |
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155 | (4) |
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159 | (1) |
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160 | (2) |
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162 | (12) |
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162 | (3) |
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165 | (4) |
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169 | (1) |
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Hydrocarbons and organic residues |
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170 | (4) |
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174 | (21) |
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174 | (2) |
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176 | (2) |
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H2O-ice: the 3 μm profile |
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178 | (3) |
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Solid CO: polar and apolar mantles |
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181 | (1) |
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Other carbon-bearing ices |
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182 | (3) |
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Nitrogen and sulphur-bearing ices |
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185 | (2) |
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187 | (3) |
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Spectropolarimetry and alignment of core-mantle grains |
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190 | (3) |
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193 | (1) |
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193 | (2) |
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Continuum and line emission |
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195 | (31) |
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Theoretical considerations |
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196 | (8) |
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Equilibrium dust temperatures |
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196 | (2) |
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FIR continuum emission from an interstellar cloud |
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198 | (2) |
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200 | (2) |
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202 | (2) |
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Galactic continuum emission |
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204 | (8) |
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204 | (1) |
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Spectral energy distribution |
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204 | (3) |
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207 | (3) |
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210 | (1) |
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Polarization and grain alignment |
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210 | (2) |
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Spectral emission features |
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212 | (10) |
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212 | (2) |
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Polycyclic aromatic hydrocarbons |
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214 | (8) |
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222 | (4) |
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224 | (1) |
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225 | (1) |
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226 | (37) |
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The formation of dust in stellar outflows |
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227 | (8) |
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Theoretical considerations |
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227 | (2) |
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The circumstellar environment |
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229 | (1) |
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230 | (2) |
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232 | (2) |
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Late stages of stellar evolution |
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234 | (1) |
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Observational constraints on stardust |
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235 | (17) |
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Infrared continuum emission |
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235 | (3) |
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Infrared spectral features |
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238 | (7) |
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245 | (2) |
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247 | (5) |
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Evolved stars as sources of interstellar grains |
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252 | (11) |
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252 | (3) |
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255 | (1) |
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256 | (1) |
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257 | (1) |
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257 | (4) |
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261 | (1) |
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261 | (2) |
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Evolution in the interstellar medium |
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263 | (32) |
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Grain surface reactions and the origin of molecular hydrogen |
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264 | (4) |
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268 | (3) |
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271 | (4) |
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272 | (1) |
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273 | (2) |
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Ice mantles: deposition and evolution |
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275 | (12) |
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Surface chemistry and hierarchical growth |
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275 | (2) |
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Depletion timescales and limits to growth |
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277 | (2) |
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Thermal and radiative processing |
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279 | (8) |
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287 | (8) |
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287 | (3) |
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290 | (1) |
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291 | (1) |
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292 | (1) |
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293 | (1) |
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293 | (2) |
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Dust in the envelopes of young stars |
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295 | (37) |
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The early phases of stellar evolution |
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296 | (10) |
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296 | (2) |
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Infrared emission from dusty envelopes |
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298 | (4) |
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Polarization and scattering |
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302 | (2) |
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Ice sublimation in hot cores |
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304 | (2) |
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306 | (6) |
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307 | (1) |
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308 | (2) |
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310 | (2) |
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Clues from the early Solar System |
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312 | (10) |
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313 | (5) |
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318 | (2) |
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320 | (2) |
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322 | (10) |
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322 | (1) |
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323 | (2) |
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Amino acids and chirality |
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325 | (3) |
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328 | (1) |
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329 | (2) |
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331 | (1) |
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331 | (1) |
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Toward a unified model for interstellar dust |
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332 | (8) |
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333 | (4) |
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333 | (2) |
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335 | (1) |
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335 | (1) |
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336 | (1) |
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336 | (1) |
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337 | (3) |
A Glossary |
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340 | (8) |
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340 | (1) |
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Physical, chemical and astrophysical terms |
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341 | (5) |
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346 | (2) |
References |
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348 | (30) |
Index |
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378 | |