| Issue |
A&A
Volume 575, March 2015
|
|
|---|---|---|
| Article Number | A95 | |
| Number of page(s) | 20 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201424969 | |
| Published online | 03 March 2015 | |
Online material
Appendix A
Gas mean molecular weight μgas, C/O ratio, and initial elemental mass yields as a function of ejecta zone for the 15 and 19 M⊙ stellar progenitors (SC13).
Ejecta temperature Tgas and number density ngas for the homogeneous, stratified SN ejecta with 15 and 19 M⊙ stellar progenitors as a function of post-explosion time and ejecta zones (SC13).
Grain size distribution function f(a) normalised to Ntot(a) as a function of radius a at day 2000 for all the dust components of the standard 15 M⊙ case.
Grain size distribution function f(a) normalised to Ntot(a) as a function of radius a at day 2000 for all the dust components of the standard 15 M⊙ case.
Grain size distribution function f(a) normalised to Ntot(a) as a function of radius a at day 2000 for forsterite, alumina, carbon, and pure silicon, and the clumpy 19 M⊙ ejecta model.
Grain size distribution function f(a) normalised to Ntot(a) as a function of radius a at day 2000 for pure-Mg, pure-Fe, iron sulphide, and silicon carbide, and the clumpy 19 M⊙ ejecta model.
© ESO, 2015
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