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http://hdl.handle.net/20.500.12386/31415
Title: | EXTraS discovery of an X-ray superflare from an L dwarf | Authors: | DE LUCA, Andrea STELZER, BEATE Burgasser, Adam J. Pizzocaro, Daniele Ranalli, Piero Raetz, Stefanie MARELLI, MARTINO Novara, Giovanni VIGNALI, CRISTIAN BELFIORE MONDONI, Andrea ESPOSITO, PAOLO FRANZETTI, PAOLO FUMANA, Marco GILLI, Roberto SALVATERRA, Ruben TIENGO, ANDREA |
Issue Date: | 2020 | Journal: | ASTRONOMY & ASTROPHYSICS | Number: | 634 | First Page: | L13 | Abstract: | We present the first detection of an X-ray flare from an ultracool dwarf of spectral class L. The event was identified in the EXTraS database of XMM-Newton variable sources, and its optical counterpart, J0331-27, was found through a cross-match with the Dark Energy Survey Year 3 release. Next to an earlier four-photon detection of Kelu-1, J0331-27 is only the second L dwarf detected in X-rays, and much more distant than other ultracool dwarfs with X-ray detections (photometric distance of 240 pc). From an optical spectrum with the VIMOS instrument at the VLT, we determine the spectral type of J0331-27 to be L1. The X-ray flare has an energy of E<SUB>X, F</SUB> ˜ 2 × 10<SUP>33</SUP> erg, placing it in the regime of superflares. No quiescent emission is detected, and from 2.5 Ms of XMM-Newton data we derive an upper limit of L<SUB>X, qui</SUB> < 10<SUP>27</SUP> erg s<SUP>-1</SUP>. The flare peak luminosity (L<SUB>X, peak</SUB> = 6.3 × 10<SUP>29</SUP> erg s<SUP>-1</SUP>), flare duration (τ<SUB>decay</SUB> ≈ 2400 s), and plasma temperature (≈16 MK) are similar to values observed in X-ray flares of M dwarfs. This shows that strong magnetic reconnection events and the ensuing plasma heating are still present even in objects with photospheres as cool as ˜2100 K. However, the absence of any other flares above the detection threshold of E<SUB>X, F</SUB> ˜ 2.5 × 10<SUP>32</SUP> erg in a total of ˜2.5 Ms of X-ray data yields a flare energy number distribution inconsistent with the canonical power law dN/dE ˜ E<SUP>-2</SUP>, suggesting that magnetic energy release in J0331-27 - and possibly in all L dwarfs - takes place predominantly in the form of giant flares. | URI: | http://hdl.handle.net/20.500.12386/31415 | URL: | https://www.aanda.org/articles/aa/full_html/2020/02/aa37163-19/aa37163-19.html | ISSN: | 0004-6361 | DOI: | 10.1051/0004-6361/201937163 | Bibcode ADS: | 2020A&A...634L..13D | Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista |
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aa37163-19.pdf | Pdf editoriale | 231.23 kB | Adobe PDF | View/Open |
aa37163-19.pdf | postprint | 214.95 kB | Adobe PDF | View/Open |
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