Diagnosis of the neutron star and its environment with X-ray astronomy

Details Diagnosis of the neutron star and its environment with X-ray astronomy Diagnosis of the neutron star and its environment with X-ray astronomy

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981plap.rept..251o&link_type=abstract

In ESA Plasma Astrophys. p 251-263 (SEE N82-20030 10-88)

Astronomy and Astrophysics

Astronomy

Crab Nebula, Japanese Space Program, Neutron Stars, Pulsars, Stellar Envelopes, X Ray Astronomy, X Ray Sources, Satellite Observation, Space Exploration, Stellar Atmospheres

Scientific paper

The physics of the neutron star, its atmosphere and its environment are discussed, relating to observational results from X-ray astronomy. The behavior of an X-ray pulsar, Vela X-1, observed with the X-ray astronomy satellite Hakucho, is considered in relation to the nature of the neutron star and its interaction with an accretion disk. X-ray bursts, also observed with the satellite, are a rich source of information for physics of the atmosphere and the plasma environment of the neutron star. The hard X-ray imaging of the Crab Nebula undertaken by balloon observation reveals the internal structure of the Crab Nebula.

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