Tidal asteroseismology: Kepler's KOI-54
We develop a general framework for interpreting and analysing high-precision light curves from eccentric stellar binaries. Although our methods are general, we focus on the recently discovered Kepler system KOI-54, a face-on binary of two A stars with e= 0.83 and an orbital period of 42 days. KOI-54...
| Main Authors: | , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
Oxford University Press
2013
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| Online Access: | http://hdl.handle.net/1721.1/76683 https://orcid.org/0000-0001-9194-2084 |