1. IE browser is NOT supported anymore. Please use Chrome, Firefox or Edge instead.
2. If you are a new user, please register to get an IHEP SSO account through https://login.ihep.ac.cn/registlight.jsp Any questions, please email us at helpdesk@ihep.ac.cn or call 88236855.
3. If you need to create a conference in the "Conferences, Workshops and Events" zone, please email us at helpdesk@ihep.ac.cn.
4. The max file size allowed for upload is 100 Mb.

A new supersoft X-ray progenitor model for the particular type Ia supernovae

23 Apr 2013, 16:40
20m
Xi'an

Xi'an

Oral Talk

Speaker

Mr Iminhaji Ablimit (.)

Description

By using a low mass supersoft source (SSS) model with magnetic confinement and Eggleton's code, we investigate the progenitors for some observed type Ia supernova (SNe Ia) with high absolute magnitude. We calculate the properties of supernova companions when the white dwarfs (WDs) of mass 1.0,1.1, and 1.2M(solar mass) grow to Chandrasekhar limit mass. We find that a low mass SSS with a magnetic WD which can confine the accreted matter in its polar caps can be the progenitor of the particular SNe Ia.

Primary author

Co-author

Prof. xiang dong Li (supervisor)

Presentation materials

There are no materials yet.