Optical Photometry of Type II-P Supernova 2004dj in NGC 2403
arXiv:astro-ph/0512526 · doi:10.1086/500972
Abstract
We present photometric data of the type II-P supernova (SN) 2004dj in NGC 2403. The multicolor light curves cover the SN from 60 to 200 days after explosion, and are measured with a set of intermediate-band filters that have the advantage of tracing the strength variations of some spectral features. The light curves show a flat evolution in the middle of the plateau phase, then decline exponentially at the late times, with a rate of 0.100.03 mag (10 days) in most of the filters. In the nebular phase, the spectral energy distribution (SED) of SN 2004dj shows a steady increase in the flux near 6600 Åand 8500 Å, which may correspond to the emission lines of H and Ca II near-IR triplet, respectively. The photometric behavior suggests that SN 2004dj is a normal SN II-P. Compared with the light curves of another typical SN II-P 1999em, we estimate the explosion date to be June 1021 UT, 2004 (JD 245316721) for SN 2004dj. We also estimate the ejected nickel mass during the explosion to be = 0.023 0.005 from two different methods, which is typical for a SN II-P. We derive the explosion energy erg, the ejecta mass , and the initial radius for the presupernova star of SN 2004dj, which are consistent with other typical SNe II-P.
arXiv comment15 pages, 9 figures, accepted for publication in AJ
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