Abstract
We present the identification of the progenitor of the Type IIP SN
2012ec in archival pre-explosion Hubble Space Telescope Wide Field
Planetary Camera 2 (WFPC2) and Advanced Camera for Surveys Wide Field
Channel F814W images. The properties of the progenitor are further
constrained by non-detections in pre-explosion WFPC2 F450W and F606W
images. We report a series of early photometric and spectroscopic
observations of SN 2012ec. The r'-band light curve shows a
plateau with M_{r^' }}=-17.0. The early spectrum is similar to the Type
IIP SN 1999em, with the expansion velocity measured at Hα
absorption minimum of -11 700 km s-1 (at 1 d post-discovery).
The photometric and spectroscopic evolution of SN 2012ec shows it to be
a Type IIP SN, discovered only a few days post-explosion (
Original language | English |
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Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 431 |
Publication status | Published - 01 Apr 2013 |
Keywords
- supernovae: general
- supernovae: individual: 2012ec
- galaxies: individual: NGC 1084