Characterizing a Dramatic ΔV ~ -9 Flare on an Ultracool Dwarf Found by the ASAS-SN Survey

February 2014 • 2014ApJ...781L..24S

Authors • Schmidt, Sarah J. • Prieto, Jose L. • Stanek, K. Z. • Shappee, Benjamin J. • Morrell, Nidia • Bardalez Gagliuffi, Daniella C. • Kochanek, C. S. • Jencson, J. • Holoien, T. W. -S. • Basu, U. • Beacom, John F. • Szczygieł, D. M. • Pojmanski, G. • Brimacombe, J. • Dubberley, M. • Elphick, M. • Foale, S. • Hawkins, E. • Mullins, D. • Rosing, W. • Ross, R. • Walker, Z.

Abstract • We analyze a ΔV ~ -9 magnitude flare on the newly identified M8 dwarf SDSS J022116.84+194020.4 (hereafter SDSSJ0221) detected as part of the All-Sky Automated Survey for Supernovae. Using infrared and optical spectra, we confirm that SDSSJ0221 is a relatively nearby (d ~ 76 pc) M8 dwarf with strong quiescent Hα emission. Based on kinematics and the absence of features consistent with low-gravity (young) ultracool dwarfs, we place a lower limit of 200 Myr on the age of SDSSJ0221. When modeled with a simple, classical flare light curve, this flare is consistent with a total U-band flare energy E_U ~ 10³⁴ erg, confirming that the most dramatic flares are not limited to warmer, more massive stars. Scaled to include a rough estimate of the emission line contribution to the V band, we estimate a blackbody filling factor of ~10%-30% during the flare peak and ~0.5%-1.6% during the flare decay phase. These filling factors correspond to flare areas that are an order of magnitude larger than those measured for most mid-M dwarf flares.

This publication is partially based on observations obtained with the Apache Point Observatory 3.5 m telescope, which is owned and operated by the Astrophysical Research Consortium.

Links

View on ADS

IPAC Authors
(alphabetical)

Jacob Jencson

Assistant Scientist