MAXI J1659-152 fading in optical

Open Access
Authors
  • D.M. Russell
  • F. Lewis
  • L. Schreuder
  • Y.J. Yang
Publication date 28-07-2011
Journal The astronomer's telegram
Volume | Issue number 3517
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract It was recently reported that the black hole candidate X-ray binary MAXI J1659-152 has faded to an X-ray flux (0.5-10 keV) of < 3.0e-13 ergs cm-2 s-1 (ATel #3506). This implies the source may be in quiescence after an outburst that lasted almost one year (GCN #11296, ATel #2873) including a late re-brightening in the last three months (ATels #3298, #3339, #3358, #3379). Here we report on recent optical observations with the two 2-m Faulkes Telescopes North and South (see ATel #2884).
Document type Article
Language English
Published at https://www.astronomerstelegram.org/?read=3517
Other links https://ui.adsabs.harvard.edu/abs/2011ATel.3517....1R/abstract
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MAXI J1659-152 fading in optical (Final published version)
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