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WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS A SMALL NEPTUNE AROUND A BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY
Title
WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS A SMALL NEPTUNE AROUND A BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY
Type
Article in International Scientific Journal
Year
2014
Authors
Van Eylen, V
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Lund, MN
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Aguirre, VS
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Arentoft, T
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Kjeldsen, H
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Albrecht, S
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Chaplin, WJ
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Isaacson, H
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Pedersen, MG
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Jessen-Hansen, J
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Tingley, B
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Christensen-Dalsgaard, J
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Aerts, C
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Campante, TL
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Bryson, ST
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