Gamma-ray observations of cygnus X-1 with the oriented scintillation spectrometer experiment

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

40 Scopus citations

Abstract

We report on ∼ 120 days of observations of Cygnus X-1 with OSSE on board the Compton Gamma Ray Observatory. Emission is detected in the range 50 keV-1 MeV, and we find evidence for a continuum of hard X-ray flux levels 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)907-914
Number of pages8
JournalAstrophysical Journal
Volume465
Issue number2 PART I
DOIs
StatePublished - Jan 1 1996

Keywords

  • Gamma rays: observations
  • Stars: individual (Cygnus X-1)
  • Stars: oscillations
  • X-rays: stars

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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