n127844SE Academic Article uri icon


  • SN 1997D in NGC 1536 is possibly the least luminous and energetic Type II supernova discovered to date. The entire light curve is subluminous, never reaching Mv = -14.65. The radioactive tail follows the 56Co decay slope. In the case of a nearly complete trapping of the -rays, the 36Ni mass derived from the tail brightness is extremely small, 0.002 M. At discovery, the spectra showed a red continuum and line velocities on the order of 1000 km s-1. The luminosity and the photospheric expansion velocity suggest that the explosion occurred about 50 days before discovery and that a plateau probably followed. Model light curves and spectra of the explosion of a 26 M star successfully fitted the observations. Low-mass models are inconsistent with the observations. The radius of the progenitor, constrained by the prediscovery upper limits, is R0 300 R. A low explosion energy of 4 1050 ergs is then required in the modeling. The strong Ba n lines in the photospheric spectra are reproduced with a solar abundance and low Teff. A scenario in which the low 56Ni mass observed in SN 1997D is due to fallback of material onto the collapsed remnant of the explosion of a 25-40 M star appears to be favored over the case of the explosion of an 8-10 M star with low 56Ni production. 1998. The American Astronomical Society. All rights resered.

published proceedings

  • Astrophysical Journal

author list (cited authors)

  • Turatto, M., Mazzali, P. A., Young, T. R., Nomoto, K., Iwamoto, K., Benetti, S., ... Sollerman, J.

publication date

  • January 1, 1998 11:11 AM