The Astrophysical Journal (Jan 2025)

The Low-redshift Lyman Continuum Survey: The Roles of Stellar Feedback and Interstellar Medium Geometry in LyC Escape

  • Sophia R. Flury,
  • Anne E. Jaskot,
  • Alberto Saldana-Lopez,
  • M. S. Oey,
  • John Chisholm,
  • Ricardo Amorín,
  • Omkar Bait,
  • Sanchayeeta Borthakur,
  • Cody Carr,
  • Henry C. Ferguson,
  • Mauro Giavalisco,
  • Matthew Hayes,
  • Timothy Heckman,
  • Alaina Henry,
  • Zhiyuan Ji,
  • Lena Komarova,
  • Florian Leclercq,
  • Alexandra Le Reste,
  • Stephan McCandliss,
  • Rui Marques-Chaves,
  • Göran Östlin,
  • Laura Pentericci,
  • Swara Ravindranath,
  • Michael Rutkowski,
  • Claudia Scarlata,
  • Daniel Schaerer,
  • Trinh Thuan,
  • Maxime Trebitsch,
  • Eros Vanzella,
  • Anne Verhamme,
  • Bingjie Wang,
  • Gábor Worseck,
  • Xinfeng Xu

DOI
https://doi.org/10.3847/1538-4357/adc305
Journal volume & issue
Vol. 985, no. 1
p. 128

Abstract

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One of the fundamental questions of cosmology is the origin and mechanism(s) responsible for the reionization of the Universe beyond z ∼ 6. Many studies have focused on Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) observations of local ( z ∼ 0.3) galaxies emitting ionizing radiation (Lyman continuum, or LyC) for insight. However, LyC measurements can depend on chance alignment of optically thin channels with the observer. In addition, low signal in the spectra of these faint LyC emitters inhibits constraints on gas geometry and stellar populations. To circumvent these limitations, we analyze stacks of a consolidated sample of HST/COS observations of the LyC in 89 galaxies at z ∼ 0.3. From fitting of the continuum, we obtain information about the underlying stellar populations, emergent LyC, and neutral interstellar medium geometry. We find that most LyC nondetections are not leaking appreciable LyC ( ${f}_{\mathrm{esc}}^{\mathrm{LyC}}$ 5%) also requires a confluence of young stars and ionizing feedback. A two-stage burst of star formation is critical to producing this optimal LyC escape scenario, and should be considered fundamental to identifying LyC emitters at the Epoch of Reionization.

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