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Conference Paper: Are the kepler near-resonance planet pairs due to tidal dissipation?

TitleAre the kepler near-resonance planet pairs due to tidal dissipation?
Authors
Lee, MHFabrycky, DLin, DNC
Issue Date2013
Citation
The 2013 Winter Conferrence of the Aspen Center for Physocs on Astrophysics, Aspen, CO., 9-15 February 2013. How to Cite?
DescriptionConference Theme: Exoplanets in Multi-body Systems in the Kepler Era
Persistent Identifierhttp://hdl.handle.net/10722/190777

 

DC FieldValueLanguage
dc.contributor.authorLee, MHen_US
dc.contributor.authorFabrycky, Den_US
dc.contributor.authorLin, DNCen_US
dc.date.accessioned2013-09-17T15:42:06Z-
dc.date.available2013-09-17T15:42:06Z-
dc.date.issued2013en_US
dc.identifier.citationThe 2013 Winter Conferrence of the Aspen Center for Physocs on Astrophysics, Aspen, CO., 9-15 February 2013.en_US
dc.identifier.urihttp://hdl.handle.net/10722/190777-
dc.descriptionConference Theme: Exoplanets in Multi-body Systems in the Kepler Era-
dc.languageengen_US
dc.relation.ispartofAspen Center for Physocs 2013 Winter Conferrence on Astrophysicsen_US
dc.titleAre the kepler near-resonance planet pairs due to tidal dissipation?en_US
dc.typeConference_Paperen_US
dc.identifier.emailLee, MH: mhlee@hku.hken_US
dc.identifier.authorityLee, MH=rp00724en_US
dc.identifier.hkuros222743en_US

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