Recent High Energy Observations of Young Neutron Stars

Details Recent High Energy Observations of Young Neutron Stars Recent High Energy Observations of Young Neutron Stars

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003head....7.5001r&link_type=abstract

American Astronomical Society, HEAD meeting #7, #50.01; Bulletin of the American Astronomical Society, Vol. 35, p.659

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations with Chandra, Newton-XMM, and RXTE of young, isolated neutron stars are increasingly giving insight into many long standing problems. Recent X-ray observations are further constraining models of high-energy emission from young pulsars and are beginning to constrain the neutron star equation of state. The identification of SGRs and AXPs as magnetars is becoming firmer, and the dividing line between these two source classes has been blurred even further. X-ray imaging and radio pulsation searches continue to discover new, energetic pulsars providing ready targets for the next generation of γ -ray telescopes.

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