Altan Baykal, Sinan K. Yerli, Sitki C. Inam, Sergei Grebenev9781402038600, 1-4020-3860-7
Neutron stars hold a central place in astrophysics, not only because they are made up of the most extreme states of the condensed matter, but also because they are, along with white dwarfs and black holes, one of the stable configurations that stars reach at the end of stellar evolution. Neutron stars posses the highest rotation rates and strongest magnetic fields among all stars. They radiate prolifically, in high energy electromagnetic radiation and in the radio band.This book is devoted to the selected lectures presented in the 6th NATO-ASI series entitled “The Electromagnetic Spectrum of Neutron Stars” in Marmaris, Turkey, on 7-18 June 2004. This ASI is devoted to the spectral properties of neutron stars. Spectral observations of neutron stars help us to understand the magnetospheric emission processes of isolated radio pulsars and the emission processes of accreting neutron stars. This volume includes spectral information from the neutron stars in broadest sense, namely neutrino and gravitational radiation along with the electromagnetic spectrum. We believe that this volume can serve as graduate level of text including the broad range of properties of neutron stars. |
Table of contents : TheElectromagneticSpectrumo1137_f.jpg……Page 1 1.pdf……Page 2 2.pdf……Page 17 3.pdf……Page 29 4.pdf……Page 46 5.pdf……Page 61 6.pdf……Page 66 7.pdf……Page 70 8.pdf……Page 82 9.pdf……Page 96 10.pdf……Page 100 11.pdf……Page 104 12.pdf……Page 117 13.pdf……Page 122 14.pdf……Page 126 15.pdf……Page 130 16.pdf……Page 145 17.pdf……Page 149 18.pdf……Page 154 19.pdf……Page 166 20.pdf……Page 171 21.pdf……Page 185 22.pdf……Page 197 23.pdf……Page 242 24.pdf……Page 246 25.pdf……Page 257 26.pdf……Page 261 27.pdf……Page 266 28.pdf……Page 281 29.pdf……Page 285 30.pdf……Page 302 31.pdf……Page 330 32.pdf……Page 335 33.pdf……Page 345 34.pdf……Page 357 35.pdf……Page 371 36.pdf……Page 376 |
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