The Physics of the Interstellar Medium, Second EditionThe book leads the advanced undergraduate through the wide range of disciplines related to an understanding of the interstellar medium and is suitable for any student studying either physics or astrophysics. The study of the interstellar medium incorporates a large range of physical More...processes on both large and small scales all of which are covered in this text. Together with the inclusion of simple models and problems at the end of each chapter this text provides a comprehensive overview and grounding in the study of the interstellar medium. |
Contents
II | 1 |
III | 5 |
IV | 6 |
V | 7 |
VI | 8 |
VII | 9 |
VIII | 12 |
IX | 16 |
LVI | 88 |
LVII | 89 |
LVIII | 92 |
LIX | 93 |
LX | 95 |
LXI | 97 |
LXII | 99 |
LXIII | 102 |
X | 21 |
XI | 24 |
XII | 25 |
XIII | 28 |
XIV | 29 |
XV | 30 |
XVI | 32 |
XVII | 35 |
XIX | 37 |
XX | 39 |
XXI | 42 |
XXII | 44 |
XXIII | 47 |
XXIV | 48 |
XXV | 49 |
XXVI | 50 |
XXVIII | 52 |
XXIX | 54 |
XXX | 55 |
XXXI | 56 |
XXXII | 57 |
XXXIII | 59 |
XXXIV | 60 |
XXXV | 61 |
XXXVI | 62 |
XXXVII | 64 |
XXXVIII | 65 |
XXXIX | 66 |
XL | 67 |
XLI | 68 |
XLII | 70 |
XLIV | 72 |
XLV | 73 |
XLVII | 75 |
XLVIII | 77 |
XLIX | 79 |
L | 80 |
LI | 81 |
LII | 84 |
LV | 87 |
LXIV | 103 |
LXV | 104 |
LXVI | 106 |
LXVII | 107 |
LXVIII | 109 |
LXIX | 112 |
LXX | 113 |
LXXII | 114 |
LXXIII | 115 |
LXXIV | 116 |
LXXV | 117 |
LXXVI | 119 |
LXXVII | 120 |
LXXVIII | 121 |
LXXIX | 122 |
LXXXI | 123 |
LXXXIII | 125 |
LXXXIV | 127 |
LXXXV | 128 |
LXXXVI | 129 |
LXXXVII | 130 |
LXXXVIII | 131 |
LXXXIX | 132 |
XC | 133 |
XCI | 134 |
XCIII | 135 |
XCIV | 136 |
XCV | 137 |
XCVI | 138 |
XCVII | 141 |
XCVIII | 143 |
XCIX | 146 |
C | 148 |
CI | 149 |
CII | 150 |
CIII | 152 |
CV | 156 |
| 161 | |
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Common terms and phrases
absorption abundances adiabatic approximately assume astronomers astrophysical bremsstrahlung bubble Chapter collisional collisions compression conservation constant continuum cooling rate cosmic ray cross-section decreases diffuse nebulae effects electron emission emitted energy levels equation equilibrium excited extinction figure flow forbidden lines frequency Galaxy gas density gas temperature grains H atoms H₂ heat Hence HII region important increases interaction interstellar clouds interstellar gas interstellar medium ionization potential ionized gas ions isothermal kinetic energy magnetic field mass material molecular cloud molecules momentum motion neutral gas number density observed occur optical oxygen P₁ particles photoionization photons plane pressure produced radiative radius rate coefficient reactions rotation shock velocity shock wave shocked gas shocked wind shows sound speed spectra spectrum star formation stellar UV stellar wind Strömgren Strömgren sphere supernova surface thermal energy thin shell timescale transition typical unit volume wavelength