Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2011-11-30
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
12 pages, 9 figures, Accepted for publication in the Astrophysical Journal
Scientific paper
We present the results of a campaign to monitor active M dwarfs using infrared spectroscopy, supplemented with optical photometry and spectroscopy. We detected 16 flares during nearly 50 hours of observations on EV Lac, AD Leo, YZ CMi, and VB8. The three most energetic flares also showed infrared emission, including the first reported detections of P\beta, P\gamma, He I 10830\AA and Br\gamma during an M dwarf flare. The strongest flare (\Delta u = 4.02 on EV Lac) showed emission from H\gamma, H\delta, He I 4471\AA, and Ca II K in the UV/blue and P\beta, P\gamma, P\delta, Br\gamma, and He I 10830\AA in the infrared. The weaker flares (\Delta u = 1.68 on EV Lac and \Delta U = 1.38 on YZ CMi) were only observed with photometry and infrared spectroscopy; both showed emission from P\beta, P\gamma, and He I 10830\AA. The strongest infrared emission line, P\beta, occurred in the active mid-M dwarfs with a duty cycle of ~3-4%. To examine the most energetic flare, we used the static NLTE radiative transfer code RH to produce model spectra based on a suite of one-dimensional model atmospheres. Using a hotter chromosphere than previous one-dimensional atmospheric models, we obtain line ratios that match most of the observed emission lines.
Hawley Suzanne L.
Hilton Eric J.
Kowalski Adam F.
Schmidt Sarah J.
Tofflemire Benjamin M.
No associations
LandOfFree
Probing the Flare Atmospheres of M dwarfs Using Infrared Emission Lines does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Probing the Flare Atmospheres of M dwarfs Using Infrared Emission Lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Probing the Flare Atmospheres of M dwarfs Using Infrared Emission Lines will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-7339