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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/014/02/0053-0063

    • Keywords

       

      Stars: Supernovae: SN1993J; techniques: photometry; stars: evolution

    • Abstract

       

      We have constructed the bolometric light curve of SN 1993J based on UBVRI(JHK) photometric data obtained from various sources and assumingAV = 0 and a distance modulus of 27.6. Effective temperatures and photosphere radius at various times have been obtained from detailed blackbody fits. The bolometric light curve shows two maxima. The short rise time to the second maximum, and the luminosities at the minimum and the second maximum are used to constrain the properties of the progenitor star. The total mass of the hydrogen envelope MH, in the star is found to be ≲ 0.2 M at the time of explosion, and the explosion ejected about 0.05 M of Ni56. Thin hydrogen envelope combined with a sufficient presupernova luminosity suggest that the exploding star was in a binary with a probable period range of 5yr ≤Porb 11yr.

    • Author Affiliations

       

      A. Ray1 K. P. Singh1 F. K. Sutaria1

      1. Tata Institute of Fundamental Research, Bombay - 400 005
    • Dates

       
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