Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas: Proceedings of the 195th Symposium of the International Astronomical Union Held at Montana State University-Bozeman, Bozeman, Montana, U.S.A., 6-10 July 1999 |
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5 pages matching ASP Conf. Ser. Vol. 161, High Energy Processes in Accreting Black Holes in this book
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Contents
The Next Generation of Highenergy Astrophysics Observatories Invited | 5 |
Recent Observations of Xray Emission from Galactic Binary Neutron | 27 |
Xray Emission Characteristics of Pulsars Invited | 49 |
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acceleration accretion disk Alfv�n Alfv�n waves ASCA Astro-E Astronomy Astrophysical Plasmas Astrophysical Plasmas IAU black hole black-hole bursts clusters component Constellation-X cooling corona cosmic rays Crab Crab Nebula density detected distribution effects electrons Emission from Astrophysical energy evolution field lines Figure flow flux frequency Galactic galaxies gamma-ray Geminga hard X-ray high-energy interaction ions jets light curve Lorentz factor luminosity M. A. Weber magnetic field magnetosphere mass Mechanisms for Emission MNRAS nebula neutron star nonthermal Observatory observed optical outer gap P. C. H. Martens pair pair production parameters particles Pavlov photons Phys Physics Plasmas IAU Symposium plerions polarization power-law produced pulsars pulse radiation radiative radio radius Ramaty reconnection region relativistic ROSAT rotation RXTE Seyfert Shibata shock simulations solar flares spectra spectrum stellar surface temperature thermal Tsuruta velocity waves X-ray binaries X-ray emission y-ray