University of Hertfordshire

High Energy Gamma Radiation From PKS 0528+134 Observed by EGRET

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Documents

  • R. Mukherjee
  • W.K. Gear
  • A.P. Marscher
  • E.M. Moore
  • J.P. Travis
  • Y. Zhang
  • E.I. Robson
  • J. A. Stevens
  • H. Terasranta
  • M. Tornikoski
  • S. Wagner
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Original languageEnglish
Title of host publicationIn: Blazar Continuum Variability - ASP Conf Series 110
PublisherAstronomical Society of the Pacific
Pages346-351
ISBN (Print)1-886733-30-9
Publication statusPublished - 1996

Abstract

A summary of EGRET observations of PKS 0528+134 is given, with special emphasis on the 1993 March observations when the source flared in gamma-rays. The flux history of PKS 0528+134 as well as spectra of the source are presented. Multiwavelength observations of PKS 0528+134 during the flare are also given. A detailed relativistic SSC jet model agrees well with the 1993 March multiwavelength spectrum. However, the data are insufficient to discriminate between this and other emission models.

Notes

Original paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific

ID: 160777