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Results 1 - 5 of 5

Overshooting in the core helium burning stage of a $30M_{odot}$ star using the $k$-$omega$ model. (arXiv:1811.06638v1 [astro-ph.SR])
- Virtual Journal - Volume 16, Issue 47 - article #5
- Yan Li, Xing-hao Chen, Hai-liang Chen
- http://arxiv.org/abs/1811.06638
Modelling nova populations in galaxies
- Virtual Journal - Volume 14, Issue 9 - article #9
- Hai-Liang Chen, T. E. Woods, L. R. Yungelson, M. Gilfanov, Zhanwen Han
- arXiv.org - Astrophysics - Volume: 2016, Issue: 26 Feb
- arXiv:1602.07849 [pdf, other]
Population synthesis of accreting white dwarfs: II. X-ray and UV emission
- Virtual Journal - Volume 13, Issue 29 - article #8
- Hai-Liang Chen, T. E. Woods, L. R. Yungelson, M. Gilfanov, Zhanwen Han
- arXiv.org - Astrophysics - Volume: 2015, Issue: 14 Aug
- arXiv:1508.03194 [pdf, ps, other]
Next generation population synthesis of accreting white dwarfs: I. Hybrid calculations using BSE + MESA
- Virtual Journal - Volume 12, Issue 16 - article #3
- Hai-Liang Chen, T. E. Woods, L. R. Yungelson, M. Gilfanov, Zhanwen Han
- arXiv.org - Astrophysics - Volume: 2014, Issue: 18 Apr
- arXiv:1404.4450 [pdf, ps, other]
A Super-Eddington Wind Scenario for the Progenitors of Type Ia Supernovae
- Virtual Journal - Volume 11, Issue 46 - article #24
- Xin Ma, Xuefei Chen, Hai-liang Chen, Pavel A. Denissenkov, and Zhanwen Han
- The Astrophysical Journal Letters - Volume: 778, Issue: 2
- View article PDF (347 KB)

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