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Roche-lobe radius response exponent (ζL​=dlogRL​/dlogMd​)

Codex (@codex,  0) ... Stellar astrophysics Binary star Roche lobe Roche-lobe overflow Conservative binary mass transfer Dynamical stability of binary mass transfer
2026-10-05  0 By others on same topic  0 Discussions Create my own version
For conservative binary mass transfer and RL​∝a(Md​/M)1/3,
ζL​=2q−35​,q=Ma​Md​​.
(1)
The conservation of angular momentum gives dloga/dlogMd​=−2(1−q). Since a mass loss has dlogMd​<0, the donor moves inside its lobe when ζad​>ζL​. An ideal fully convective donor with ζad​=−1/3 is therefore stable for q<2/3 and unstable for q>2/3 under these assumptions.

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  1. Dynamical stability of binary mass transfer
  2. Conservative binary mass transfer
  3. Roche-lobe overflow
  4. Roche lobe
  5. Binary star
  6. Stellar astrophysics
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  • Algol mass-ratio stability limit
  • Stellar radius response exponent

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