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Study of the spectral characteristics of unidentified galactic EGRET sources. Are they pulsar-like?

  • M. Merck*
  • , D. L. Bertsch
  • , B. L. Dingus
  • , J. A. Esposito
  • , C. E. Fichtel
  • , J. M. Fierro
  • , R. C. Hartman
  • , S. D. Hunter
  • , G. Kanbach
  • , D. A. Kniffen
  • , Y. C. Lin
  • , H. A. Mayer-Hasselwander
  • , P. P. Michelson
  • , C. Von Montigny
  • , A. Mücke
  • , R. Mukherjee
  • , P. L. Nolan
  • , M. Pohl
  • , E. Schneid
  • , P. Sreekumar
  • D. J. Thompson, T. D. Willis
*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

A spectral study of unidentified galactic EGRET sources was performed. The derived spectra are compared to the spectra of pulsars to test the hypothesis, that a significant fraction of these sources are Geminga like radio-quiet pulsars (Yadigaroglu and Romani 1995). Most of the sources show significantly different spectra than expected under this hypothesis. Of those with spectra consistent with typical pulsar spectra, four are positionally consistent with young spin-powered radio pulsars leaving only very few Geminga type candidates in the sample.

Original languageEnglish
Pages (from-to)465-469
Number of pages5
JournalAstronomy and Astrophysics Supplement Series
Volume120
Issue number4
Publication statusPublished - 1996

All Science Journal Classification (ASJC) codes

  • General Physics and Astronomy

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