First Millimeter Flares Detected from Epsilon Eridani with ALMA

TL;DR

This paper reports the first detection of millimeter flares from a Sun-like star, Epsilon Eridani, revealing large, rapid flares with brightness surpassing solar flares, using archival ALMA data.

Contribution

It presents the first observation of millimeter flares from a Sun-like star, expanding understanding of stellar flare phenomena at these wavelengths.

Findings

Detected three large millimeter flares from Epsilon Eridani.

Largest flare had a peak flux density of 28 mJy and lasted 9 seconds.

Flares were significantly brighter than the star's quiescent state and solar flares.

Abstract

We report the detection of three large millimeter flaring events from the nearby Sun-like, $\epsilon$ Eridani, found in archival ALMA 12m and ACA observations at 1.33 mm taken from 2015 January 17-18 and 2016 October 24-November 23, respectively. This is the first time that flares have been detected from a Sun-like star at millimeter wavelengths. The largest flare among our data was detected in the ALMA observations on 2015 January 17 from 20:09:10.4-21:02:49.3 (UTC) with a peak flux density of 28 $\pm$ 7 mJy and a duration of 9 sec. The peak brightness of the largest flare is $ 3.4 \pm 0.9 \times 10^{14}$ erg s$^{-1}$Hz$^{-1}$, a factor of $>50\times$ times brighter than the star's quiescent luminosity and $>10\times$ brighter than solar flares observed at comparable wavelengths. We find changes in the spectral index (F$_\nu\propto\nu^\alpha$) at the flare peak, with $\alpha$ = 1.81 $\pm$ 1.94 and a lower limit on the fractional linear polarization $|Q/I| = $ 0.08 $\pm$ 0.12. This positive spectral index is more similar to millimeter solar flares, differing from M dwarf flares also detected at millimeter wavelengths that exhibit steeply negative spectral indices.