The Color Excesses of Type Ia Supernovae from Single-Degenerate Channel Model

Details The Color Excesses of Type Ia Supernovae from Single-Degenerate Channel Model The Color Excesses of Type Ia Supernovae from Single-Degenerate Channel Model

2009-07-16

arxiv.org/abs/0907.2753v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

11 pages, 4 figures, accepted for publication in RAA

Scientific paper

Single Degenerate model is the most widely accepted progenitor model of type Ia supernovae (SNe Ia), in which a carbon-oxygen white dwarf (CO WD) accretes hydrogen-rich material from a main sequence or a slightly evolved star (WD +MS) to increase its mass, and explodes when its mass approaches the Chandrasekhar mass limit. During the mass transfer phase between the two components, an optically thick wind may occur and the material lost as the wind may exist as circumstellar material (CSM). Searching the CSM around progenitor star is helpful to discriminate different progenitor models of SNe Ia. Meanwhile, the CSM is a source of color excess.The purpose of this paper is to study the color excess produced from the single-degenerate progenitor model with optically thick wind, and reproduce the distribution of color excesses of SNe Ia. Meng et al. (2009) systemically carried out binary evolution calculation of the WD +MS systems for various metallicities and showed the parameters of the systems before Roche lobe overflow and at the moment of supernova explosion in Meng & Yang (2009). With the results of Meng et al. (2009), we calculate the color excesses of SNe Ia at maximum light via a simple analytic method.We reproduces the distribution of color excesses of SNe Ia by our binary population synthesis approach if the velocity of the optically thick wind is taken to be of order of magnitude of 10 km s$^{\rm -1}$. However, if the wind velocity is larger than 100 km s$^{\rm -1}$, the reproduction is bad.

Affiliated with

Also associated with

No associations

Rating

The Color Excesses of Type Ia Supernovae from Single-Degenerate Channel Model 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 The Color Excesses of Type Ia Supernovae from Single-Degenerate Channel Model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Color Excesses of Type Ia Supernovae from Single-Degenerate Channel Model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-621031