Ítems similars

• SN 2023ixf: interaction signatures in the spectrum at 445 days
  per: Folatelli, Gastón, et al.
  Publicat: (2025)
• Progenitor mass and ejecta asymmetry of SN 2023ixf from nebular spectroscopy
  per: Ferrari, Lucía, et al.
  Publicat: (2024)
• Diversity in hydrogen-rich envelope mass of type II supernovae (I): $V$-band light curve modeling
  per: Fang, Qiliang, et al.
  Publicat: (2024)
• Progenitor and explosion properties of SN 2023ixf estimated based on a light-curve model grid of Type II supernovae
  per: Moriya, Takashi J., et al.
  Publicat: (2024)
• Discovery of young, oxygen-rich supernova remnants in PHANGS-MUSE galaxies
  per: Kravtsov, Timo, et al.
  Publicat: (2024)