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|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|
Chaplin, William J.
et al, Various
Van Eylen, V.
|Publisher:||Institute of Physics Publishing|
|Citation:||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, The Astrophysical Journal, vol.782, 1, 2014,pp 1-13|
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|Type:||C1 - Refereed Journal articles|
|Appears in Collections:||University of Sydney Research Outputs|
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