Inward emission in pulsar magnetosphere

Details Inward emission in pulsar magnetosphere Inward emission in pulsar magnetosphere

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..801..265d&link_type=abstract

ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP Conference Proceedings, Volume 801, pp. 265-271 (2005).

Astronomy and Astrophysics

Astrophysics

Pulsars, Stellar Atmospheres, Stellar Magnetism, X-Ray Sources (Astronomical), Ultraviolet Sources (Astronomical), Pulsars, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation

Scientific paper

We discuss theoretical arguments and observational evidence for the existence of inward emission in pulsar magnetosphere. We show that the new soft components in the X-ray/UV pulse profile of the Vela pulsar can be interpreted in terms of the inward emission from the same outer magnetospheric regions that are thought to be responsible for the outward gamma-ray emission observed above 100 MeV. In the radio band, inward emission provides a way to interpret the main-pulse/interpulse anticorrelation in B1822-09 as well as the locations of emission and absorption features in the pulse profile of B0950+08.

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