The Largest M Dwarf Flares from ASAS-SN

The All-sky Automated Survey for Supernovae (ASAS-SN) is the only project in existence to scan the entire sky in optical light approximately every day, reaching a depth of g ∼ 18 mag. Over the course of its first 4 yr of transient alerts (2013-2016), ASAS-SN observed 53 events classified as likely M...

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Bibliographic Details

Published in:	The Astrophysical journal Vol. 876; no. 2; pp. 115 - 133
Main Authors:	Schmidt, Sarah J., Shappee, Benjamin J., van Saders, Jennifer L., Stanek, K. Z., Brown, Jonathan S., Kochanek, C. S., Dong, Subo, Drout, Maria R., Frank, Stephan, Holoien, T. W.-S., Johnson, Sean, Madore, Barry F., Prieto, J. L., Seibert, Mark, Seidel, Marja K., Simonian, Gregory V. A.
Format:	Journal Article
Language:	English
Published:	Philadelphia The American Astronomical Society 10-05-2019 IOP Publishing
Subjects:	Astrophysics Emissions Flare stars H alpha line Light curve Outbursts Red dwarf stars Sky surveys (astronomy) Spectroscopy stars: chromospheres stars: late-type stars: low-mass Stellar flares Supernovae T Tauri stars
Online Access:	Get full text
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