Is SN 2006X from a WD + MS system with optically thick wind?
arXiv:0910.1915 · doi:10.1016/j.newast.2009.09.008
Abstract
The single-degenerate channel is widely accepted as the progenitors of type Ia supernovae (SNe Ia). Following the work of Meng, Chen and Han (2009), we reproduced the birth rate and age of supernovae like SN 2006X by the single-degenerate model (WD + MS) with an optically thick wind, which may imply that the progenitor of SN 2006X is a WD + MS system.
10 pages, 2 figures, accepted for publication in NewA
References in corpus (10)
- Optical and Near-Infrared Observations of the Highly Reddened, Rapidly Expanding Type Ia Supernova 2006X in M100
- Variable Sodium Absorption in a Low-Extinction Type Ia Supernova
- Young and Massive Binary Progenitors of Type Ia Supernovae and Their Circumstellar Matter
- The single-degenerate channel for the progenitor of type Ia supernovae with different metallicities
- Evolving to Type Ia Supernovae with Short Delay Times
- A single-degenerate model for the progenitor of the Type Ia supernova 2002ic
- Companion Stars of Type Ia Supernovae
- On the progenitors of super-Chandrasekhar mass type Ia supernovae
- Evolving to type Ia supernovae with long delay time
- An Alternative Symbiotic Channel to Type Ia Supernovae