Tenma observation of the X-ray pulsar 4U1626-67

Details Tenma observation of the X-ray pulsar 4U1626-67 Tenma observation of the X-ray pulsar 4U1626-67

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..375k&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

2

Neutron Stars, Pulsars, X Ray Binaries, X Ray Sources, Dwarf Stars, Energy Spectra, Field Strength, Stellar Magnetic Fields

Scientific paper

Energy-dependent pulse profiles from the X-ray pulsar 4U1626-67, observed with Tenma in May 1983, were studied using an anisotropic radiation transfer model in an accretion column on a strongly magnetized neutron star. The result indicates that the strength of the magnetic field is about 8×1012G at the surface of the neutron star.

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