Abstract
We have found and analysed 16 multipeaked type-I bursts from the
neutron-star low-mass X-ray binary 4U 1636 - 53 with the Rossi X-ray
Timing Explorer (RXTE). One of the bursts is a rare quadruple-peaked
burst that was not previously reported. All 16 bursts show a multipeaked
structure not only in the X-ray light curves but also in the bolometric
light curves. Most of the multipeaked bursts appear in observations
during the transition from the hard to the soft state in the
colour-colour diagram. We find an anticorrelation between the second
peak flux and the separation time between two peaks. We also find that
in the double-peaked bursts the peak-flux ratio and the temperature of
the thermal component in the pre-burst spectra are correlated. This
indicates that the double-peaked structure in the light curve of the
bursts may be affected by enhanced accretion rate in the disc, or
increased temperature of the neutron star.
Original language | English |
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Pages (from-to) | 168-178 |
Number of pages | 11 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 501 |
Issue number | 1 |
DOIs | |
Publication status | Published - 1-Jan-2021 |
Keywords
- stars: individual: 4U 1636 - 53
- X-rays: binaries
- X-rays: bursts
- EXOSAT OBSERVATIONS
- IRON LINE
- OSCILLATIONS
- EVOLUTION
- EMISSION
- PHASE