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Search for linear polarization in gamma-ray sources - possible evidence for the Vela pulsar

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/166182· OSTI ID:7129527
The use of the azimuthal distribution of planes containing e(+)/e(-) pairs from high-energy photon materialization to investigate the nature of gamma-ray sources is discussed. Analytical work done on COS B data for bright COS B sources (Vela, Crab, and Geminga) and for a reference background region is presented along with results which are indicative of a low-chance-probability anisotropy effect for Vela. The case for the Vela pulsar is studied in more detail, starting from its pulsation properties and from a polarization interpretation of the observed anisotropy. A possible physical interpretation of the results is given in the context of pulsar gamma-ray emission, and requirements for future gamma-ray telescopes derived from COS B experience are examined. 29 references.
Research Organization:
CNR, Istituto di Fisica Cosmica, Milan (Italy)
OSTI ID:
7129527
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 327; ISSN ASJOA
Country of Publication:
United States
Language:
English