Search NASA⌕ Search

NASA NTRS · 19810027019

Repeatable, multiple-peaked structure in Type I X-ray bursts

Abstract

A distinct, identifiable, multiple-peaked structure has been observed in Type I X-ray bursts from three sources. At energies below 6 keV, the light curves look like typical Type I bursts. At higher energies, the burst is double-peaked, with both the depth of the dip and the separation between the peaks increasing with energy. A light curve of the energy-integrated intensity shows no distinct double peak, suggesting that only a single energy release occurs. Blackbody fits to the evolving burst spectra yield changing radii and temperatures, inversely correlated, during the early part of the burst. The physical interpretation of these changes is uncertain. Burst decay spectra yield relatively constant radii with decreasing temperatures. It is proposed that Compton scattering may be responsible for the dips in the higher-energy light curves by shifting photons to lower energies.

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Hoffman, J. A., Cominsky, L., Lewin, W. H. G.. 1980-08-15. Repeatable, multiple-peaked structure in Type I X-ray bursts. https://ntrs.nasa.gov/citations/19810027019

Cite the original work for its findings. Save a collection to share your selection of sources.