The Electromagnetic Spectrum of Neutron Stars

  • Altan Baykal
  • Sinan K. Yerli
  • Sitki C. Inam
  • Sergei Grebenev

Part of the NATO Science Series II. Mathematics, Physics and Chemistry book series (NAII, volume 210)

Table of contents

  1. Front Matter
    Pages i-xvii
  2. Formation of Neutron Stars

    1. Chris L. Fryer, Aimee Hungerford
      Pages 3-14
    2. Patrick Slane
      Pages 15-30
  3. Neutron Star Structure and Magnetic Field

    1. J. Gil, Y. Gupta, J. Kijak, M. Sendyk
      Pages 75-78
    2. U. Geppert, M. Kueker, D. Page
      Pages 79-82
    3. Andrea Passamonti, Marco Bruni, Leonardo Gualtieri, Carlos F. Sopuerta
      Pages 83-86
  4. Neutrino Astrophysics

    1. Francis Halzen
      Pages 89-101
    2. Joachim Moortgat, Jan Kuijpers
      Pages 103-106
    3. Chunglee Kim, Vassiliki Kalogera, Duncan R. Lorimer, Mia Ihm, Krzysztof Belczynski
      Pages 107-114
    4. Aimee L. Hungerford, Christopher L. Fryer, Aristotle Socrates, Omer Blaes
      Pages 111-114
  5. Cooling and Atmospheres of Neutron Stars

    1. J.E. Trümper
      Pages 117-131
    2. K. Yavuz Eksi, M. Ali Alpar
      Pages 137-140
    3. Matthew van Adelsberg, Dong Lai, Alexander Y. Potekhin
      Pages 141-144
  6. Pulsars

    1. Nichi D’Amico
      Pages 147-160
    2. D. R. Lorimer
      Pages 161-172

About these proceedings

Introduction

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.

Keywords

Accretion Gravity astronomy astrophysics stellar

Editors and affiliations

  • Altan Baykal
    • 1
  • Sinan K. Yerli
    • 1
  • Sitki C. Inam
    • 2
  • Sergei Grebenev
    • 3
  1. 1.Middle East Technical UniversityAnkaraTurkey
  2. 2.Baskent UniversityAnkaraTurkey
  3. 3.Space Research Institute (IKI)MoscowRussia

Bibliographic information

  • DOI https://doi.org/10.1007/1-4020-3861-5
  • Copyright Information Springer 2005
  • Publisher Name Springer, Dordrecht
  • eBook Packages Physics and Astronomy
  • Print ISBN 978-1-4020-3859-4
  • Online ISBN 978-1-4020-3861-7
  • Series Print ISSN 1568-2609
  • About this book