The Astrophysical Journal Letters (Jan 2023)

SN 2023ixf in Messier 101: Photo-ionization of Dense, Close-in Circumstellar Material in a Nearby Type II Supernova

  • W. V. Jacobson-Galán,
  • L. Dessart,
  • R. Margutti,
  • R. Chornock,
  • R. J. Foley,
  • C. D. Kilpatrick,
  • D. O. Jones,
  • K. Taggart,
  • C. R. Angus,
  • S. Bhattacharjee,
  • L. A. Braff,
  • D. Brethauer,
  • A. J. Burgasser,
  • F. Cao,
  • C. M. Carlile,
  • K. C. Chambers,
  • D. A. Coulter,
  • E. Dominguez-Ruiz,
  • C. B. Dickinson,
  • T. de Boer,
  • A. Gagliano,
  • C. Gall,
  • H. Gao,
  • E. L. Gates,
  • S. Gomez,
  • M. Guolo,
  • M. R. J. Halford,
  • J. Hjorth,
  • M. E. Huber,
  • M. N. Johnson,
  • P. R. Karpoor,
  • T. Laskar,
  • N LeBaron,
  • Z. Li,
  • Y. Lin,
  • S. D. Loch,
  • P. D. Lynam,
  • E. A. Magnier,
  • P. Maloney,
  • D. J. Matthews,
  • M. McDonald,
  • H.-Y. Miao,
  • D. Milisavljevic,
  • Y.-C. Pan,
  • S. Pradyumna,
  • C. L. Ransome,
  • J. M. Rees,
  • A. Rest,
  • C. Rojas-Bravo,
  • N. R. Sandford,
  • L. Sandoval Ascencio,
  • S. Sanjaripour,
  • A. Savino,
  • H. Sears,
  • N. Sharei,
  • S. J. Smartt,
  • E. R. Softich,
  • C. A. Theissen,
  • S. Tinyanont,
  • H. Tohfa,
  • V. A. Villar,
  • Q. Wang,
  • R. J. Wainscoat,
  • A. L. Westerling,
  • E. Wiston,
  • M. A. Wozniak,
  • S. K. Yadavalli,
  • Y. Zenati

DOI
https://doi.org/10.3847/2041-8213/acf2ec
Journal volume & issue
Vol. 954, no. 2
p. L42

Abstract

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We present UV and/or optical observations and models of SN 2023ixf, a type II supernova (SN) located in Messier 101 at 6.9 Mpc. Early time ( flash ) spectroscopy of SN 2023ixf, obtained primarily at Lick Observatory, reveals emission lines of H i , He i/ii , C iv , and N iii/iv/v with a narrow core and broad, symmetric wings arising from the photoionization of dense, close-in circumstellar material (CSM) located around the progenitor star prior to shock breakout. These electron-scattering broadened line profiles persist for ∼8 days with respect to first light, at which time Doppler broadened the features from the fastest SN ejecta form, suggesting a reduction in CSM density at r ≳ 10 ^15 cm. The early time light curve of SN 2023ixf shows peak absolute magnitudes (e.g., M _u = −18.6 mag, M _g = −18.4 mag) that are ≳2 mag brighter than typical type II SNe, this photometric boost also being consistent with the shock power supplied from CSM interaction. Comparison of SN 2023ixf to a grid of light-curve and multiepoch spectral models from the non-LTE radiative transfer code CMFGEN and the radiation-hydrodynamics code HERACLES suggests dense, solar-metallicity CSM confined to r = (0.5–1) × 10 ^15 cm, and a progenitor mass-loss rate of $\dot{M}={10}^{-2}\,{M}_{\odot }$ yr ^−1 . For the assumed progenitor wind velocity of v _w = 50 km s ^−1 , this corresponds to enhanced mass loss (i.e., superwind phase) during the last ∼3–6 yr before explosion.

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