X-ray re-brightening of the accreting millisecond X-ray pulsar IGR J17379-3747

J. van den Eijnden, N. Degenaar, T. Russell, R. Wijnands, J. V. Hernandez Santisteban, D. M. Russell, A. AlMannaei, D. Maitra, A. W. Shaw, C. O. Heinke, G. R. Sivakoff, T. Maccarone, J. Miller-Jones, M. Armas Padilla, A. Bahramian

Research output: Book/ReportOther report

Abstract

IGR J17379-3747 is a neutron star low-mass X-ray binary, identified as an accreting millisecond X-ray pulsar by the detection of 468 Hz pulsations by NICER (Atel #11507).
Original languageEnglish
PublisherThe Astronomer's Telegram (ATel)
DOIs
Publication statusPublished - 9 Apr 2018

Publication series

NameThe Astronomer's Telegram
No.11520

Keywords

  • Neutron Star
  • Transient
  • Pulsar

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