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Table · dataset · 2026

Analysis of AGB and post-AGB wind density using the ISW model

Listed in Teesside University Research Data Repository

The radial density profiles presented in this dataset were calculated using the Interacting Stellar Winds (ISW) model for the slow stellar wind associated with the Asymptotic Giant Branch (AGB) phase and the fast stellar wind generated during the post-AGB phase.

Description

Simulations were performed in MATLAB using built-in numerical and visualization functions and standard stellar wind parameters based on the values proposed by Kwok et al. (1977).

The FastWind_Post-AGB.csv and SlowWindAGB.csv files contain the radial distance and density values for each wind, while SlowWind_FastWind_Comparison.csv provides a direct comparison between both winds.

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Where it is published

Catalogue records · 1

Topics

From keywords
Astronomy & Astrophysics · Earth & Environmental Science · Mathematics & Statistics
Provenance · 1 source records, 8 field assertions
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Teesside University Research Data Repositoryoai:data.mendeley.com/p2s97ws6ds.115 h agoJSON v1
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concepts[field].local:field:astronomymapping · researchdata tees ac ukconnector:researchdata_tees_ac_uk@1.0.0
concepts[field].local:field:earth-environmentalmapping · researchdata tees ac ukconnector:researchdata_tees_ac_uk@1.0.0
concepts[field].local:field:mathematics-statisticsmapping · researchdata tees ac ukconnector:researchdata_tees_ac_uk@1.0.0
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