Is SN 2006X from a WD + MS system with optically thick wind?

Details Is SN 2006X from a WD + MS system with optically thick wind? Is SN 2006X from a WD + MS system with optically thick wind?

2009-10-10

arxiv.org/abs/0910.1915v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

10 pages, 2 figures, accepted for publication in NewA

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Is SN 2006X from a WD + MS system with optically thick wind? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Is SN 2006X from a WD + MS system with optically thick wind?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Is SN 2006X from a WD + MS system with optically thick wind? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-620515