Phase Lag and Coherence Function of X-ray emission from Black Hole Candidate XTE J1550-564

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

To appear in ApJ Letters

Scientific paper

10.1086/312520

We report the results from measuring the phase lag and coherence function of X-ray emission from black hole candidate (BHC) XTE J1550-564. These X-ray temporal properties have been recognized to be increasingly important in providing important diagnostics of the dynamics of accretion flows around black holes. For XTE J1550-564, we found significant hard lag --- the X-ray variability in high energy bands {\em lags} behind that in low energy bands --- associated both with broad-band variability and quasi-periodic oscillation (QPO). However, the situation is more complicated for the QPO: while hard lag was measured for the first harmonic of the signal, the fundamental component showed significant {\em soft} lag. Such behavior is remarkably similar to what was observed of microquasar GRS 1915+105. The phase lag evolved during the initial rising phase of the 1998 outburst. The magnitude of both the soft and hard lags of the QPO increases with X-ray flux, while the Fourier spectrum of the broad-band lag varies significantly in shape. The coherence function is relatively high and roughly constant at low frequencies, and begins to drop almost right after the first harmonic of the QPO. It is near unity at the beginning and decreases rapidly during the rising phase. Also observed is that the more widely separated the two energy bands are the less the coherence function between the two. It is interesting that the coherence function increases significantly at the frequencies of the QPO and its harmonics. We discuss the implications of the results on the models proposed for BHCs.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Phase Lag and Coherence Function of X-ray emission from Black Hole Candidate XTE J1550-564 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Phase Lag and Coherence Function of X-ray emission from Black Hole Candidate XTE J1550-564, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Phase Lag and Coherence Function of X-ray emission from Black Hole Candidate XTE J1550-564 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-719959

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.