Gamma ray observations of Cygmis X-1 with OSSE

B. F. Phlips*, G. V. Jung, M. D. Leising, J. E. Grove, W. N. Johnson, R. L. Kinzer, R. A. Kroeger, J. D. Kurfess, M. S. Strickman, D. A. Grabelsky, S. M. Matz, W. R. Purcell, M. P. Ulmer, K. McNaron-Brown

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

4 Scopus citations

Abstract

We report on ∼120 days of observations of Cygnus X-1 with OSSE onboard the Compton Observatory. Emission is detected in the range 50 keV to 1 MeV, and we find evidence for a continuum of hard X-ray spectra over a broad range of fluxes rather than the existence of distinct flux states. Comparisons of the source spectra with various theoretical models show that an exponentially truncated power law best describes the average spectrum in the OSSE energy band. Although we have measured a new minimum in the hard X-ray flux from the source, no evidence was found for either a broad 1 MeV feature or a narrow 511 keV line previously reported in association with a low flux state. Upper limits on such emission features are an order of magnitude lower than earlier reported detections. The 5.6-day periodicity of the source measured at optical wavelengths was not detected with a sensitivity to the rms modulation fraction of 5% in the 60-140 keV energy band.

Original languageEnglish (US)
Pages (from-to)155-158
Number of pages4
JournalAstronomy and Astrophysics Supplement Series
Volume120
Issue number4
StatePublished - Dec 1 1996

Keywords

  • Cyg x-1 - Black hole physics
  • Gamma rays
  • Individual
  • Observations - Stars

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Fingerprint Dive into the research topics of 'Gamma ray observations of Cygmis X-1 with OSSE'. Together they form a unique fingerprint.

Cite this