New Primary Mechanisms for the Synthesis of Rare Be 9 in Early Supernovae

Banerjee, Projjwal; Qian, Yong-Zhong; Haxton, W. C.; Heger, Alexander

doi:10.1103/PhysRevLett.110.141101

Title: New Primary Mechanisms for the Synthesis of Rare ${}^{9}{Be}$ in Early Supernovae

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Authors:: Banerjee, Projjwal; Qian, Yong-Zhong; Haxton, W. C.; Heger, Alexander

Publication Date:: 2013-04-01

Sponsoring Org.:: USDOE

OSTI Identifier:: 1103994

Resource Type:: Publisher's Accepted Manuscript

Journal Name:: Physical Review Letters

Additional Journal Information:: Journal Volume: 110; Journal Issue: 14; Journal ID: ISSN 0031-9007

Publisher:: American Physical Society

Country of Publication:: United States

Language:: English

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                    Banerjee, Projjwal, Qian, Yong-Zhong, Haxton, W. C., and Heger, Alexander. New Primary Mechanisms for the Synthesis of Rare Be 9 in Early Supernovae.  United States: N. p., 2013. 
Web.  doi:10.1103/PhysRevLett.110.141101.

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                    Banerjee, Projjwal, Qian, Yong-Zhong, Haxton, W. C., & Heger, Alexander. New Primary Mechanisms for the Synthesis of Rare Be 9 in Early Supernovae.  United States.  https://doi.org/10.1103/PhysRevLett.110.141101

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                    Banerjee, Projjwal, Qian, Yong-Zhong, Haxton, W. C., and Heger, Alexander. Mon .  
"New Primary Mechanisms for the Synthesis of Rare Be 9 in Early Supernovae".  United States.  https://doi.org/10.1103/PhysRevLett.110.141101.

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@article{osti_1103994,

  title        = {New Primary Mechanisms for the Synthesis of Rare Be 9 in Early Supernovae},

  author       = {Banerjee, Projjwal and Qian, Yong-Zhong and Haxton, W. C. and Heger, Alexander},

  abstractNote = {},

  doi          = {10.1103/PhysRevLett.110.141101},

  journal      = {Physical Review Letters},

  number       = 14,

  volume       = 110,

  place        = {United States},

  year         = {2013},

  month        = {4}

}

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Title: New Primary Mechanisms for the Synthesis of Rare Be 9 in Early Supernovae

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Title: New Primary Mechanisms for the Synthesis of Rare ${}^{9}{Be}$ in Early Supernovae