Log in

NuSTAR and AstroSat observations of thermonuclear X-ray bursts with short-recurrence times in 4U 1636−536

  • Binaries
  • Published:
Journal of Astrophysics and Astronomy Aims and scope Submit manuscript

Abstract

We report results from the spectro-timing analysis of the atoll source 4U 1636−536 observed with NuSTAR and AstroSat during its hard spectral state. In three observations of 207 ks total exposure, we identify 31 thermonuclear X-ray bursts including five doublets and a triplet. Recurrence time as short as 3.8 min is seen in one of the doublets. To the best of our knowledge, this is the shortest recurrence time known for this source. Our time-averaged spectroscopy during the bursts indicates the presence of an additional power-law or a blackbody component in a few cases, perhaps due to varying temperatures during bursts or plausible deviation from ideal blackbody behavior; however, it is difficult to probe this using the time-resolved spectroscopy owing to limited statistics. Time-resolved bursts are well fit using an absorbed blackbody model with temperatures varying between 1.7 and 2.2 keV. Burst oscillations around 581 Hz are detected with 3\(\sigma \) confidence during the decay phase in two of the X-ray bursts. One of the burst oscillations is seen at 582 Hz, a frequency observed during the 2001 superburst in this source.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Subscribe and save

Springer+ Basic
EUR 32.99 /Month
  • Get 10 units per month
  • Download Article/Chapter or Ebook
  • 1 Unit = 1 Article or 1 Chapter
  • Cancel anytime
Subscribe now

Buy Now

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Figure 1
Figure 2
Figure 3
Figure 4
Figure 5
Figure 6
Figure 7
Figure 8
Figure 9

Similar content being viewed by others

References

Download references

Acknowledgments

AB and PR acknowledge the financial support of ISRO under AstroSat archival Data utilization program (No. DS-2B-13013(2)/4/2019-Sec.2). AB is grateful to the Royal Society, UK and to SERB (Science and Engineering Research Board), India and is supported by an INSPIRE Faculty Grant (DST/INSPIRE/04/2018/001265) by the Department of Science and Technology (DST), Government of India. This research has made use of the NuSTAR data analysis software (NuSTARDAS) jointly developed by the ASI Science Center (ASDC, Italy) and the California Institute of Technology (Caltech, USA). The data for this research have been provided by the High Energy Astrophysics Science Archive Research Centre (HEASARC) and the Indian Space Science Data Centre (ISSDC). We thank the anonymous referee for important inputs towards the improvement of the paper.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to PINAKI ROY.

Additional information

This article is part of the Special Issue on “Astrophysical Jets and Observational Facilities: A National Perspective”.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

ROY, P., BERI, A. & MONDAL, A.S. NuSTAR and AstroSat observations of thermonuclear X-ray bursts with short-recurrence times in 4U 1636−536. J Astrophys Astron 43, 45 (2022). https://doi.org/10.1007/s12036-022-09825-8

Download citation

  • Received:

  • Accepted:

  • Published:

  • DOI: https://doi.org/10.1007/s12036-022-09825-8

Keywords

Navigation