Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...327l..13s&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 327, April 1, 1988, p. L13-L16.
Astronomy and Astrophysics
Astrophysics
16
Periodic Variations, Stellar Oscillations, Time Lag, X Ray Binaries, X Ray Spectra, Compton Effect, Electron Plasma, Optical Thickness, Stellar Models
Scientific paper
Time lags in the 0.4-5-Hz quasi-periodic oscillations (QPOs) of the rapid burster are investigated using two Exosat observations. Different QPO modes were noted during long type 2 bursts and in the persistent emission. The 1-5 keV X-ray signal lagged behind the 5-21-keV signal by 7.6 + or - 2.1 ms in the persistent emission QPO with frequencies of greater than 3.6 Hz. The fractional strength of the QPO was found to increase with photon energy during the persistent emission interval. The results provide evidence for a soft lag in QPOs which is suggested to be due to spectral softening during each QPO cycle.
Haberl Franck
Lewin Walter H. G.
Paradijs Jan van
Parmar Arvind N.
Stella Luigi
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