The Astrophysical Journal (Jan 2024)

Final Moments. II. Observational Properties and Physical Modeling of Circumstellar-material-interacting Type II Supernovae

  • W. V. Jacobson-Galán,
  • L. Dessart,
  • K. W. Davis,
  • C. D. Kilpatrick,
  • R. Margutti,
  • R. J. Foley,
  • R. Chornock,
  • G. Terreran,
  • D. Hiramatsu,
  • M. Newsome,
  • E. Padilla Gonzalez,
  • C. Pellegrino,
  • D. A. Howell,
  • A. V. Filippenko,
  • J. P. Anderson,
  • C. R. Angus,
  • K. Auchettl,
  • K. A. Bostroem,
  • T. G. Brink,
  • R. Cartier,
  • D. A. Coulter,
  • T. de Boer,
  • M. R. Drout,
  • N. Earl,
  • K. Ertini,
  • J. R. Farah,
  • D. Farias,
  • C. Gall,
  • H. Gao,
  • M. A. Gerlach,
  • F. Guo,
  • A. Haynie,
  • G. Hosseinzadeh,
  • A. L. Ibik,
  • S. W. Jha,
  • D. O. Jones,
  • D. Langeroodi,
  • N LeBaron,
  • E. A. Magnier,
  • A. L. Piro,
  • S. I. Raimundo,
  • A. Rest,
  • S. Rest,
  • R. Michael Rich,
  • C. Rojas-Bravo,
  • H. Sears,
  • K. Taggart,
  • V. A. Villar,
  • R. J. Wainscoat,
  • X-F. Wang,
  • A. R. Wasserman,
  • S. Yan,
  • Y. Yang,
  • J. Zhang,
  • W. Zheng

DOI
https://doi.org/10.3847/1538-4357/ad4a2a
Journal volume & issue
Vol. 970, no. 2
p. 189

Abstract

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We present ultraviolet/optical/near-infrared observations and modeling of Type II supernovae (SNe II) whose early time ( δ t < 2 days) spectra show transient, narrow emission lines from shock ionization of confined ( r < 10 ^15 cm) circumstellar material (CSM). The observed electron-scattering broadened line profiles (i.e., IIn-like) of H i , He i/ii , C iv , and N iii/iv/v from the CSM persist on a characteristic timescale ( t _IIn ) that marks a transition to a lower-density CSM and the emergence of Doppler-broadened features from the fast-moving SN ejecta. Our sample, the largest to date, consists of 39 SNe with early time IIn-like features in addition to 35 “comparison” SNe with no evidence of early time IIn-like features, all with ultraviolet observations. The total sample includes 50 unpublished objects with a total of 474 previously unpublished spectra and 50 multiband light curves, collected primarily through the Young Supernova Experiment and Global Supernova Project collaborations. For all sample objects, we find a significant correlation between peak ultraviolet brightness and both t _IIn and the rise time, as well as evidence for enhanced peak luminosities in SNe II with IIn-like features. We quantify mass-loss rates and CSM density for the sample through the matching of peak multiband absolute magnitudes, rise times, t _IIn , and optical SN spectra with a grid of radiation hydrodynamics and non-local thermodynamic equilibrium radiative-transfer simulations. For our grid of models, all with the same underlying explosion, there is a trend between the duration of the electron-scattering broadened line profiles and inferred mass-loss rate: ${t}_{\mathrm{IIn}}\approx 3.8[\dot{M}/$ (0.01 M _⊙ yr ^−1 )] days.

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