Tidal evolution of massive, eccentric binary systems: Effects of resonance locking
Contrary to what is generally assumed, resonant tidal interaction with gravity modes seems a common phenomenon during the evolution of massive eccentric binary systems. This is because non-resonant low order retrograde orbital harmonics drive weak high order harmonics up into resonance until the res...
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| Format: | Conference item |
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2001
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| _version_ | 1797104804049190912 |
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| author | Savonije, G Witte, MG |
| author_facet | Savonije, G Witte, MG |
| author_sort | Savonije, G |
| collection | OXFORD |
| description | Contrary to what is generally assumed, resonant tidal interaction with gravity modes seems a common phenomenon during the evolution of massive eccentric binary systems. This is because non-resonant low order retrograde orbital harmonics drive weak high order harmonics up into resonance until the resonant interaction counterbalances the driving and the prograde harmonic gets locked. This frequently occurring near-resonant tidal interaction gives rise to strongly enhanced tidal evolution whereby large orbital eccentricities decay to small values in only a few million years in systems with orbital periods less than about 10 days. |
| first_indexed | 2024-03-07T06:38:41Z |
| format | Conference item |
| id | oxford-uuid:f887a048-7c47-4269-8ebf-e8da63c847d7 |
| institution | University of Oxford |
| last_indexed | 2024-03-07T06:38:41Z |
| publishDate | 2001 |
| record_format | dspace |
| spelling | oxford-uuid:f887a048-7c47-4269-8ebf-e8da63c847d72022-03-27T12:50:57ZTidal evolution of massive, eccentric binary systems: Effects of resonance lockingConference itemhttp://purl.org/coar/resource_type/c_5794uuid:f887a048-7c47-4269-8ebf-e8da63c847d7Symplectic Elements at Oxford2001Savonije, GWitte, MGContrary to what is generally assumed, resonant tidal interaction with gravity modes seems a common phenomenon during the evolution of massive eccentric binary systems. This is because non-resonant low order retrograde orbital harmonics drive weak high order harmonics up into resonance until the resonant interaction counterbalances the driving and the prograde harmonic gets locked. This frequently occurring near-resonant tidal interaction gives rise to strongly enhanced tidal evolution whereby large orbital eccentricities decay to small values in only a few million years in systems with orbital periods less than about 10 days. |
| spellingShingle | Savonije, G Witte, MG Tidal evolution of massive, eccentric binary systems: Effects of resonance locking |
| title | Tidal evolution of massive, eccentric binary systems: Effects of resonance locking |
| title_full | Tidal evolution of massive, eccentric binary systems: Effects of resonance locking |
| title_fullStr | Tidal evolution of massive, eccentric binary systems: Effects of resonance locking |
| title_full_unstemmed | Tidal evolution of massive, eccentric binary systems: Effects of resonance locking |
| title_short | Tidal evolution of massive, eccentric binary systems: Effects of resonance locking |
| title_sort | tidal evolution of massive eccentric binary systems effects of resonance locking |
| work_keys_str_mv | AT savonijeg tidalevolutionofmassiveeccentricbinarysystemseffectsofresonancelocking AT wittemg tidalevolutionofmassiveeccentricbinarysystemseffectsofresonancelocking |