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Can scallop-shell stars trap dust in their magnetic fields?

Abstract:

One of the puzzles to have emerged from the Kepler and TESS missions is the existence of unexplained dips in the lightcurves of a small fraction of rapidly-rotating M dwarfs in young open clusters and star-forming regions. We present a theoretical investigation of one possible explanation - that these are caused by dust clouds trapped in the stellar magnetic fields. The depth and duration of the observed dips allow us to estimate directly the linear extent of the dust clouds and their distanc...

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Publication status:
In press
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/stac3302

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Institution:
University of Oxford
Division:
MPLS
Department:
Earth Sciences
Oxford college:
Exeter College
Role:
Author
ORCID:
0000-0001-5842-6985
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Role:
Author
ORCID:
0000-0002-1466-5236
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Role:
Author
ORCID:
0000-0002-8863-7828
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Role:
Author
ORCID:
0000-0002-4996-6901
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Role:
Author
ORCID:
0000-0001-5541-2887
More from this funder
Funding agency for:
Donati, J-F
Grant:
#740651 NewWorlds
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Funding agency for:
Sanderson, H
Grant:
NE/S007474/1
More from this funder
Funding agency for:
Jardine, M
Cameron, AC
Grant:
ST/R000824/1
RSE Cormack Vacation Scholarship, Royal Society of Edinburgh More from this funder
Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Publication date:
2022-11-12
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Language:
English
Keywords:
Pubs id:
1310780
Local pid:
pubs:1310780
Deposit date:
2022-11-30

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