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The MUSCLES Treasury Survey. V. FUV flares on active and inactive M dwarfs

Abstract:

M dwarf stars are known for their vigorous flaring. This flaring could impact the climate of orbiting planets, making it important to characterize M dwarf flares at the short wavelengths that drive atmospheric chemistry and escape. We conducted a far-ultraviolet flare survey of six M dwarfs from the recent MUSCLES (Measurements of the Ultraviolet Spectral Characteristics of Low-mass Exoplanetary Systems) observations, as well as four highly active M dwarfs with archival data. When comparing a...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.3847/1538-4357/aae2bd

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ORCID:
0000-0001-5646-6668
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ORCID:
0000-0002-1002-3674
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ORCID:
0000-0002-1176-3391
Schneider, C More by this author
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ORCID:
0000-0003-2631-3905
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Hubble Space Telescope More from this funder
University of Colorado More from this funder
Publisher:
Institute of Physics Publisher's website
Journal:
Astrophysical Journal Journal website
Volume:
867
Issue:
1
Pages:
71
Publication date:
2018-11-01
Acceptance date:
2018-09-18
DOI:
EISSN:
1538-4357
ISSN:
0004-637X
Pubs id:
pubs:951332
URN:
uri:1b142cbc-3384-4246-a304-8a2ace4e10aa
UUID:
uuid:1b142cbc-3384-4246-a304-8a2ace4e10aa
Local pid:
pubs:951332

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