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Optical evolution of Swift J174510.8-262411 suggests the compact jet is fading, radio flare imminent?

  • D. M. Russell
  • , F. Lewis
  • , Carole Mundell
  • , A. Tripp
  • , T. Belloni
  • , P Curran
  • , H. Krimm
  • , D. Maitra
  • , J. C. A. Miller-Jones
  • , G. R. Sivakoff
  • INAF - Osservatorio Astronomico di Brera
  • NASA Goddard Space Flight Center
  • Universities Space Research Association

Research output: Contribution to journal › Article › peer-review

Abstract

We report on optical monitoring observations of the outburst of the black hole candidate X-ray binary Swift J174510.8-262411 (Sw J1725-26; e.g. GCN #13744; ATel #4383; #4393; #4394; #4450) with the Faulkes Telescope South (FTS; located at Siding Spring, Australia) in SDSS i'-band, Bessel R and Bessel V filters. The first FTS images were acquired just 19 minutes after the original Swift BAT trigger.
Original languageEnglish
JournalThe Astronomer's Telegram
Volume4456
Publication statusPublished - Oct 2012

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