Thermonuclear X-ray bursts in rapid succession in 4U 1636-536 with AstroSat-LAXPC
Abstract
We present results from an observation of the low-mass X-ray binary 4U 1636-536 obtained with the LAXPC instrument aboard AstroSat. The observations of 4U 1636-536 made during the performance verification phase of AstroSat showed seven thermonuclear X-ray bursts in a total exposure of ∼65 ks over a period of about two consecutive days. Moreover, the light curve of 4U 1636-536 revealed the presence of a rare triplet of X-ray bursts, having a wait time of about 5.5 min between the second and the third bursts. We also present results from time-resolved spectroscopy performed during these seven X-ray bursts. In addition, we have also detected a transient quasi-periodic oscillation at ∼5 Hz. However, we did not find any evidence of kilo-hertz quasi-periodic oscillations and/or X-ray burst oscillations, perhaps due to the hard spectral state of the source during this observation.
- Publication:
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Monthly Notices of the Royal Astronomical Society
- Pub Date:
- February 2019
- DOI:
- arXiv:
- arXiv:1811.10030
- Bibcode:
- 2019MNRAS.482.4397B
- Keywords:
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- accretion;
- accretion discs;
- stars: neutron;
- X-rays: binaries;
- X-rays: bursts;
- X-rays: individual: 4U 1636—536;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- Accepted for publication in MNRAS