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1. update Kamlah+ 2022 reference from arXiv link to formal link 2. add useful badges to make the repo look more formal on GitHub
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name: autotest namelist and old | ||
name: Demo simulation test | ||
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on: | ||
push: | ||
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This is Nbody6++GPU - Beijing version, an N-body star cluster simulation code, maintained by Rainer Spurzem (spurzem/at/nao.cas.cn) and team. | ||
[![autotest status](https://github.com/nbody6ppgpu/Nbody6PPGPU-beijing/actions/workflows/autotest.yml/badge.svg)](https://github.com/nbody6ppgpu/Nbody6PPGPU-beijing/actions/workflows/autotest.yml) | ||
[![Paper](https://badgen.net/badge/NASA%20ads/1999PASP..111.1333A/blue?icon=https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg)](https://ui.adsabs.harvard.edu/abs/1999PASP..111.1333A/abstract) | ||
[![Paper](https://badgen.net/badge/NASA%20ads/1999JCoAM.109..407S/blue?icon=https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg)](https://ui.adsabs.harvard.edu/abs/1999JCoAM.109..407S/abstract) | ||
[![Paper](https://badgen.net/badge/NASA%20ads/2005MNRAS.363..293H/blue?icon=https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg)](https://ui.adsabs.harvard.edu/abs/2005MNRAS.363..293H/abstract) | ||
[![Paper](https://badgen.net/badge/NASA%20ads/2012MNRAS.424..545N/blue?icon=https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg)](https://ui.adsabs.harvard.edu/abs/2012MNRAS.424..545N/abstract) | ||
[![Paper](https://badgen.net/badge/NASA%20ads/2015MNRAS.450.4070W/blue?icon=https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg)](https://ui.adsabs.harvard.edu/abs/2015MNRAS.450.4070W/abstract) | ||
[![Paper](https://badgen.net/badge/NASA%20ads/2022MNRAS.511.4060K/blue?icon=https://ui.adsabs.harvard.edu/styles/img/transparent_logo.svg)](https://ui.adsabs.harvard.edu/abs/2022MNRAS.511.4060K/abstract) | ||
<!-- [![Paper](https://badgen.net/badge/arXiv/0000.0000/green?icon=https://static.arxiv.org/static/browse/0.3.4/images/arxiv-logo-one-color-white.svg )](https://arxiv.org/abs/xxxxx) --> | ||
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This is Nbody6++GPU - Beijing version, an N-body star cluster simulation code, maintained by Rainer Spurzem ([email protected]) and team. | ||
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The code is an offspring of Sverre Aarseth's direct N-body codes see www.sverre.com . | ||
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@@ -109,7 +118,7 @@ or ask any question in [our discussion](https://github.com/nbody6ppgpu/Nbody6PPG | |
- https://ui.adsabs.harvard.edu/abs/2005MNRAS.363..293H/abstract (Hurley+ on SSE/BSE, earlier references therein) | ||
- https://ui.adsabs.harvard.edu/abs/2012MNRAS.424..545N/abstract (Nitadori+: NBODY6GPU) | ||
- https://ui.adsabs.harvard.edu/abs/2015MNRAS.450.4070W/abstract (Wang+: NBODY6++GPU) | ||
- https://ui.adsabs.harvard.edu/abs/2021arXiv210508067K/abstract (Kamlah+: More on current stellar evol.) | ||
- https://ui.adsabs.harvard.edu/abs/2022MNRAS.511.4060K/abstract (Kamlah+: More on current stellar evol.) | ||
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# For contributors | ||
```git clone -b dev [email protected]:nbody6ppgpu/Nbody6PPGPU-beijing``` | ||
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