Direct Analysis of Spectra of the Unusual Type Ib Supernova 2005bf

Synthetic spectra generated with the parameterized supernova synthetic spectrum code SYNOW are compared to spectra of the unusual Type Ib supernova 2005bf. We confirm the discovery by Folatelli et al. that very early spectra (∼30 days before maximum light) contain both photospheric‐velocity (∼8000 km s−1) features of He i, Ca ii, and Fe ii, and detached high‐velocity (∼14,000 km s−1) features of Hα, Ca ii, and Fe ii. An early spectrum of SN 2005bf is an almost perfect match to a near–maximum‐light spectrum of the Type Ib SN 1999ex. Although these two spectra were at very different times with respect to maximum light (20 days before maximum for SN 2005bf and 5 days after for SN 1999ex), they were for similar times after explosion—about 20 days for SN 2005bf and 24 days for SN 1999ex. The almost perfect match clinches the previously suggested identification of Hα in SN 1999ex and supports the proposition that many if not all Type Ib supernovae eject a small amount of hydrogen. The earliest available spectrum of SN 2005bf resembles a near–maximum‐light spectrum of the Type Ic SN 1994I. These two spectra were also at different times with respect to maximum light (32 days before maximum for SN 2005bf and 4 days before for SN 1994I) but at similar times after explosion—about 8 days for SN 2005bf and 10 days for SN 1994I. The resemblance motivates us to consider a reinterpretation of the spectra of Type Ic supernovae, involving coexisting photospheric‐velocity and high‐velocity features. The implications of our results for the geometry of the SN 2005bf ejecta, which has been suggested as being grossly asymmetric, are briefly discussed.