数据链接：
官方服务：
资源简介：
Core collapse models of helium stars at Z=0.04
应用场景：
创建时间：
2020-09-02
相关数据集
Nucleosynthesis Yields from Boccioli & Roberti (2026)
Isotopic and Elemental Yields from neutrino-driven core-collapse supernova simulations described in Boccioli & Roberti (2026) of three different sets of stellar evolution calculations (WH07, LC18, and
Zenodo2026-03-30 更新50
Stellar Mass Black Hole Formation and Multimessenger Signals from Three-dimensional Rotating Core-collapse Supernova Simulations
Gravitational waveforms from Pan et al. (2021) . They are the 40 solar mass model from Woosley & Heger 2007 with differentinitial rotational speeds: Model NR: Omega_0 = 0.0 rad/secModel SR: Omega_0
Zenodo2024-09-11 更新30
Reproducibility package for: "Nuclear Neural Networks: Emulating late burning stages in Core Collapse Supernova Progenitors"
Reproducibility package for: "Nuclear Neural Networks: Emulating late burning stages in Core Collapse Supernova Progenitors". It contains mesa stellar models used to determine the parameter space of t
NIAID Data Ecosystem20
Simulations of supernova explosions
We present radiation-hydrodynamic simulations of core-collapse supernova (SN) explosions, artificially generated by driving a piston at the base of the envelope of a rotating or...
B2FIND50
Constraining properties of the next nearby core-collapse supernova with multi-messenger signals: multi-messenger signals
1D FLASH simulations with STIR, for alpha_lambda = 1.23, 1.25, and 1.27. Run with SFHo EOS, M1 with 12 energy groups. For more information on these simulations, see Warren, Couch, O'Connor, & Moro
Zenodo2020-05-13 更新20
