Padova stellar model grid

Figshare2016-01-19 更新2026-04-08 收录

恒星与亚恒星演化模型

等时线计算

数据链接：

https://figshare.com/articles/dataset/Padova_stellar_model_grid/1247204/1 数据链接链接失效反馈

官方服务：

资源简介：

Padova stellar model grid to be used by 'isochrones' python module (by automatic download).

创建时间：

2014-11-20

POPSTAR with Chabrier IMF

恒星与亚恒星演化模型

星族合成

PopStar Evolutionary synthesis models. Using IMF from Chabrier (2003). This grid of Single Stellar Populations covers a wide range in both, age and metallicity. The models use...

B2FIND60

Pair-instability supernovae models

恒星与亚恒星演化模型

不稳定性超新星

Both recent observations and stellar evolution models suggest that pair-instability supernovae (PISNe) could occur in the local Universe, at metallicities below Z_{sun}_/3....

B2FIND40

Grids of stellar models III.

恒星与亚恒星演化模型

天体物理学

Stellar evolutionary models with mass loss and moderate overshooting at metallicity Z = 0.004 in the 0.80 to 120 M{sun} range are presented. They complete the set of grids...

B2FIND30

Stellar evolution tracks comparing turbulent pressure driven mass loss and the de Jager mass-loss rates

恒星与亚恒星演化模型

恒星质量损失

The uploaded files provide a series of stellar evolution tracks with initial masses from 16 to 20 \(M_\odot\). The two sets of tracks compare the evolution of stars evolved on the red supergiant branc

Zenodo2022-06-16 更新40

Energy source and pre-explosion progenitor evolution of SuperLuminous Supernovae

超新星爆发机制

恒星与亚恒星演化模型

With bolometric luminosities reaching Lvirgul10^45 erg/sec, the new class of SuperLuminous Supernovae (SLSNe) outshine ordinary SNe a factor 100 and represent thedeath of the most massive stars in our

ESA Earth Online30

Padova stellar model grid

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