---
res:
  bibo_abstract:
  - Although planets have been found orbiting binary systems, whether they can survive
    binary interactions is debated. While the tightest-orbit binaries should host
    the most dynamically stable and long-lived circumbinary planetary systems, they
    are also the systems that are expected to experience mass transfer, common envelope
    evolution, or stellar mergers. In this study, we explore the effect of stable
    non-conservative mass transfer on the dynamical evolution of circumbinary planets.
    We present a new script that seamlessly integrates binary evolution data from
    the 1D binary stellar evolution code MESA into the N-body simulation code REBOUND.
    This integration framework enables a comprehensive examination of the dynamical
    evolution of circumbinary planets orbiting mass-transferring binaries, while simultaneously
    accounting for the detailed stellar structure evolution. In addition, we introduce
    a recalibration method to mitigate numerical errors from updates of binary properties
    during the system's dynamical evolution. We construct a reference binary model
    in which a 2.21M⊙ star loses its hydrogen-rich envelope through non-conservative
    mass transfer to the 1.76M⊙ companion star, creating a 0.38M⊙ subdwarf. We find
    the tightest stable orbital separation for circumbinary planets to be ≃2.5 times
    the binary separation after mass transfer. Accounting for tides by using the interior
    stellar structure, we find that tidal effects become apparent after the rapid
    mass transfer phase and start to fade away during the latter stage of the slow
    mass transfer phase. Our research provides a new framework for exploring circumbinary
    planet dynamics in interacting binary systems.@eng
  bibo_authorlist:
  - foaf_Person:
      foaf_givenName: Zepei
      foaf_name: Xing, Zepei
      foaf_surname: Xing
  - foaf_Person:
      foaf_givenName: Santiago
      foaf_name: Torres Rodriguez, Santiago
      foaf_surname: Torres Rodriguez
      foaf_workInfoHomepage: http://www.librecat.org/personId=a8df4360-4328-11ee-8f1a-e502d0c83fc2
    orcid: 0000-0002-3150-8988
  - foaf_Person:
      foaf_givenName: Ylva Louise Linsdotter
      foaf_name: Götberg, Ylva Louise Linsdotter
      foaf_surname: Götberg
      foaf_workInfoHomepage: http://www.librecat.org/personId=d0648d0c-0f64-11ee-a2e0-dd0faa2e4f7d
    orcid: 0000-0002-6960-6911
  - foaf_Person:
      foaf_givenName: Alessandro A.
      foaf_name: Trani, Alessandro A.
      foaf_surname: Trani
  - foaf_Person:
      foaf_givenName: Valeriya
      foaf_name: Korol, Valeriya
      foaf_surname: Korol
  - foaf_Person:
      foaf_givenName: Jorge
      foaf_name: Cuadra, Jorge
      foaf_surname: Cuadra
  bibo_doi: 10.1093/mnras/stae2820
  bibo_issue: '1'
  bibo_volume: 537
  dct_date: 2025^xs_gYear
  dct_identifier:
  - UT:001400731500001
  dct_isPartOf:
  - http://id.crossref.org/issn/0035-8711
  - http://id.crossref.org/issn/1365-2966
  dct_language: eng
  dct_publisher: Oxford University Press@
  dct_title: 'Combining REBOUND and MESA: Dynamical evolution of planets orbiting
    interacting binaries@'
...