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Dwarkadas, V.V. and Gruszko, J. (2011) What Are Published X-Ray Light Curves Telling Us about Young Supernova Expansion? Monthly Notices of the Royal Astronomical Society, 419, 1515-1524.
https://doi.org/10.1111/j.1365-2966.2011.19808.x

has been cited by the following article:

• TITLE: Swift XRT Analysis of Type II-P Supernova SN 2008ij

  AUTHORS: SH. M. Shehata, Ahmed M. Fouad, R. M. Samir, A. A. Shaker

  KEYWORDS: X-Ray Core Collapse Supernova, Swift (XRT) Observations

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.14 No.3, September 10, 2024

  ABSTRACT: This study investigates the X-ray properties and evolution of Type II supernovae (SNe II) observed by Swift, examining variations among supernovae and exploring their X-ray characteristics over time. We present the first X-ray study of the Type IIp supernova SN 2008ij using data from the Swift X-ray mission. This investigation focuses on its spectral properties, identifying an X-ray flux of 1.20 (+0.11, −0.10) × 10−13 erg/cm2/s and a plasma temperature of 4.76 (+1.22, −0.83) keV. Our study marks an advancement in understanding SN 2008ij, providing crucial results into its X-ray emission characteristics. These results lay the groundwork for future studies of Type IIp supernovae, offering a foundation for exploring their evolutionary and physical processes.