Abstract
A source coincident with the position of the type IIb supernova (SN) 2008ax is identified in pre-explosion Hubble Space Telescope (HST) Wide Field Planetary Camera 2 observations in three optical filters. We identify and constrain two possible progenitor systems: (i) a single massive star that lost most of its hydrogen envelope through radiatively driven mass-loss processes, prior to exploding as a helium-rich Wolf-Rayet star with a residual hydrogen envelope, and (ii) an interacting binary in a low-mass cluster producing a stripped progenitor. Late time, high-resolution observations along with detailed modelling of the SN will be required to reveal the true nature of this progenitor star.
Original language | English |
---|---|
Pages (from-to) | L5-L9 |
Number of pages | 5 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 391 |
Issue number | 1 |
DOIs | |
Publication status | Published - Nov 2008 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science