Nickel Bubble Expansion in Type Ia Supernovae: Adiabatic Solutions | Zendy

ChihYueh Wang | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

Nickel Bubble Expansion in Type Ia Supernovae: Adiabatic Solutions

Author(s) -

ChihYueh Wang

Publication year - 2008

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/591217

Subject(s) - ejecta , physics , supernova , radius , astrophysics , shell (structure) , radioactive decay , detonation , adiabatic process , bubble , radiative transfer , explosive material , mechanics , atomic physics , thermodynamics , materials science , chemistry , composite material , computer security , organic chemistry , quantum mechanics , computer science

This paper presents hydrodynamical and radiation-hydrodynamical simulationsof the nickel bubble effect in Type Ia supernovae, comparison of results toself-similar solutions, and application to observations of Type Ia supernovaremnants, with a particular emphasis on Tycho's SNR.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research