University of Hertfordshire

From the same journal

From the same journal

By the same authors

Documents

  • 1812.00016v1

    Accepted author manuscript, 847 KB, PDF-document

  • Steve Mairs
  • Bhavana Lalchand
  • Geoffrey C. Bower
  • Jan Forbrich
  • Graham S. Bell
  • Gregory J. Herczeg
  • Doug Johnstone
  • Wen-Ping Chen
  • Jeong-Eun Lee
  • Alvaro Hacar
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Original languageEnglish
JournalThe Astrophysical Journal
Journal publication date30 Nov 2018
StateAccepted/In press - 30 Nov 2018

Abstract

The binary T Tauri system JW 566 in the Orion Molecular Cloud underwent an energetic, short-lived flare observed at submillimetre wavelengths by the SCUBA-2 instrument on 26 November 2016 (UT). The emission faded by nearly 50% during the 31 minute integration. The simultaneous source fluxes averaged over the observation are 500 +/- 107 mJy/beam at 450 microns and 466 +/- 47 mJy/beam at 850 microns. The 850 micron flux corresponds to a radio luminosity of $L_{\nu}=8\times10^{19}$ erg/s/Hz, approximately one order of magnitude brighter (in terms of $\nu L_{\nu}$) than that of a flare of the young star GMR-A, detected in Orion in 2003 at 3mm. The event may be the most luminous known flare associated with a young stellar object and is also the first coronal flare discovered at sub-mm wavelengths. The spectral index between 450 microns and 850 microns of $\alpha = 0.11$ is broadly consistent with non-thermal emission. The brightness temperature was in excess of $6\times10^{4}$ K. We interpret this event to be a magnetic reconnection that energised charged particles to emit gyrosynchrotron/synchrotron radiation.

Notes

Accepted in ApJ. 16 pages (single column), 6 figures

ID: 15796836