SIMBAD references

We present photometry and spectroscopy of the Type IIP supernova (SN IIP) 2009bw in UGC 2890 from a few days after the outburst to 241 d. The light curve of SN 2009bw during the photospheric phase is similar to that of normal SNe IIP but with a brighter peak and plateau ({img} mag, {img} mag). The luminosity drop from the photospheric to the nebular phase is one of the fastest ever observed, ∼ 2.2 mag in about 13 d. The radioactive tail of the bolometric light curve indicates that the amount of ejected ⁵⁶Ni is ≈ 0.022 M_☉. The photospheric spectra reveal high-velocity lines of Hα and Hβ until about 105 d after the shock breakout, suggesting a possible early interaction between the SN ejecta and pre-existent circumstellar material, and the presence of CNO elements. By modelling the bolometric light curve, ejecta expansion velocity and photospheric temperature, we estimate a total ejected mass of ∼ 8-12 M_☉, a kinetic energy of ∼ 0.3 foe and an initial radius of ∼ 3.6-7 {x} 10¹³ cm.