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An Optically Discovered Outburst from XTE J1859+226

Bellm, Eric C. (author)
Wang, Yuankun (author)
van Roestel, Jan (author)
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Phillipson, Rebecca A. (author)
Coughlin, Michael W. (author)
Tomsick, John A. (author)
Groom, Steven L. (author)
Healy, Brian (author)
Purdum, Josiah (author)
Rusholme, Ben (author)
Sollerman, Jesper, 1968- (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Bealo, Peter (author)
Lora, Stefano (author)
Muyllaert, Eddy (author)
Peretto, Ivo (author)
Schwendeman, Erik J. (author)
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 (creator_code:org_t)
2023
2023
English.
In: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 956:1
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Using the Zwicky Transient Facility, in 2021 February we identified the first known outburst of the black hole X-ray transient XTE J1859+226 since its discovery in 1999. The outburst was visible at X-ray, UV, and optical wavelengths for less than 20 days, substantially shorter than its full outburst of 320 days in 1999, and the observed peak luminosity was 2 orders of magnitude lower. Its peak bolometric luminosity was only 2 × 1035 erg s−1, implying an Eddington fraction of about 3 × 10−4. The source remained in the hard spectral state throughout the outburst. From optical spectroscopy measurements we estimate an outer disk radius of 1011 cm. The low observed X-ray luminosity is not sufficient to irradiate the entire disk, but we observe a surprising exponential decline in the X-ray light curve. These observations highlight the potential of optical and infrared synoptic surveys to discover low-luminosity activity from X-ray transients.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

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