X-ray Emission Characteristics of Pulsars

Details X-ray Emission Characteristics of Pulsars X-ray Emission Characteristics of Pulsars

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000iaus..195...49b&link_type=abstract

Highly Energetic Physical Processes and Mechanisms for Emission from Astrophysical Plasmas, Proceedings of IAU Symposium #195, h

Astronomy and Astrophysics

Astronomy

7

Scientific paper

Recent X-ray observatories such as ROSAT, ASCA, RXTE, BeppoSAX, and Chandra have achieved important progress in neutron star and pulsar astronomy. The identification of Geminga as a rotation-powered pulsar, the discovery of X-ray emission from millisecond pulsars, and the identification of cooling neutron stars are only a few of the fascinating results. In the following, I will give a brief review on the X-ray emission properties of rotation-powered pulsars and their wind nebulae.

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