{
  "abstract": "There are indications that the Large Magellanic Cloud (LMC) hosts a central supermassive black hole (SMBH), yet no direct detection exists: one reason is that its present-day location need not necessarily coincide with the photometric or kinematic centers. Here we frame a dynamical targeting problem and predict the present-day sky location of the LMC SMBH. We model the recent LMC-Small Magellanic Cloud (SMC) interaction, which induces a bar-disk offset, and integrate SMBH orbits within a realistic, time-dependent LMC-SMC-Milky Way (MW) potential. We show that the MW tidal field at present epoch exceeds that of the SMC by at least an order of magnitude, setting a preferred direction for coherent, vertical low-amplitude displacements, while the disk asymmetry drives in-plane offsets. Projecting onto the observed LMC frame, the mean of our predicted SMBH probability distribution is located at $(α,δ)=(80.23^{\\circ},-69.55^{\\circ})$, with a $1σ$ confidence ellipse having semi-major and semi-minor axes of $(a,b)=(1.34^{\\circ},0.56^{\\circ})$, respectively. This mean is $\\sim6$ arcminutes north of the adopted dynamical center, while the mode coincides with the dynamical center and lies well within the $1σ$ confidence region. Furthermore, all literature estimates of the LMC center considered here fall within the $2σ$ confidence region. This provides a concrete, testable target for ongoing and upcoming spectroscopic surveys, transforming the search for the LMC SMBH from an unconstrained problem into a focused observational strategy.",
  "abstract_shown": true,
  "affiliations": [],
  "article_type": null,
  "arxiv": "2609.16177",
  "author_total": 5,
  "authors": [
    {
      "name": "Robin Chisholm"
    },
    {
      "name": "Elena D'Onghia"
    },
    {
      "name": "Niv Drory"
    },
    {
      "name": "Andrew Fox"
    },
    {
      "name": "Noam Libeskind"
    }
  ],
  "bibtex": "https://research.draconitic.com/paper/46m8ndw0nafn0.bib",
  "cited_by": 0,
  "doi": "10.48550/arxiv.2609.16177",
  "fulltext_url": null,
  "id": "46m8ndw0nafn0",
  "issns": [],
  "landing_url": "https://arxiv.org/abs/2609.16177",
  "language": null,
  "licence": "CC-BY-4.0",
  "licence_label": "CC BY 4.0",
  "licence_source": "article",
  "licence_url": "http://creativecommons.org/licenses/by/4.0/",
  "metadata_licence": "CC0-1.0",
  "native_subjects": [
    [
      "arxiv",
      "astro-ph.GA"
    ]
  ],
  "openalex": null,
  "pdf_url": "https://arxiv.org/pdf/2609.16177",
  "pmcid": null,
  "pmid": null,
  "published": "2026-09-14",
  "publisher": null,
  "ris": "https://research.draconitic.com/paper/46m8ndw0nafn0.ris",
  "sources": [
    {
      "first_seen": "2026-10-30T12:21:41Z",
      "native_id": "2609.16177",
      "source": "arxiv",
      "url": "https://arxiv.org/abs/2609.16177"
    }
  ],
  "subjects": [
    {
      "field": "astronomy",
      "origin": "arxiv:astro-ph.GA",
      "subfield": "galaxies"
    }
  ],
  "title": "The Missing Black Hole in the Large Magellanic Cloud: A Dynamical Prediction for Its Present-Day Location",
  "title_text": "The Missing Black Hole in the Large Magellanic Cloud: A Dynamical Prediction for Its Present-Day Location",
  "type": "preprint",
  "updated_at": "2026-10-30T12:21:41Z",
  "url": "https://research.draconitic.com/paper/46m8ndw0nafn0",
  "venue": "arXiv",
  "versions": []
}