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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

AuthID
P-00R-40M

Author(s)

Van Eylen, V

Lund, MN

Albrecht, S

Isaacson, H

Pedersen, MG

Jessen Hansen, J

Tingley, B

Christensen Dalsgaard, J

Aerts, C

Campante, TL

Bryson, ST

Document Type

Article

Year published

2014

Published

in ASTROPHYSICAL JOURNAL, ISSN: 0004-637X

Volume: 782, Issue: 1, Pages: 14 (13)

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Publication Identifiers

DOI: 10.1088/0004-637x/782/1/14

SCOPUS: 2-s2.0-84893186280

Wos: WOS:000331848200014

Source Identifiers

ISSN: 0004-637X

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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

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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

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