A NICER Thermonuclear Burst from the Millisecond X-Ray Pulsar SAX J1808.4-3658

Bult P., Jaisawal G. K., Guver T., Strohmayer T. E., Altamirano D., Arzoumanian Z., ...More

ASTROPHYSICAL JOURNAL LETTERS, vol.885, no.1, 2019 (SCI-Expanded) identifier identifier

  • Publication Type: Article / Article
  • Volume: 885 Issue: 1
  • Publication Date: 2019
  • Doi Number: 10.3847/2041-8213/ab4ae1
  • Journal Name: ASTROPHYSICAL JOURNAL LETTERS
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Istanbul University Affiliated: Yes

Abstract

The Neutron Star Interior Composition Explorer (NICER) has extensively monitored the 2019 August outburst of the 401 Hz millisecond X-ray pulsar SAX J1808.4-3658. In this Letter, we report on the detection of a bright helium-fueled Type I X-ray burst. With a bolometric peak flux of (2.3 +/- 0.1) x 10(-7) erg s(-1) cm(-2), this was the brightest X-ray burst among all bursting sources observed with NICER to date. The burst shows a remarkable two-stage evolution in flux, emission lines at 1.0 and 6.7 keV, and burst oscillations at the known pulsar spin frequency, with approximate to 4% fractional sinusoidal amplitude. We interpret the burst flux evolution as the detection of the local Eddington limits associated with the hydrogen and helium layers of the neutron star envelope. The emission lines are likely associated with Fe, due to reprocessing of the burst emission in the accretion disk.