Spectroscopy of P30 and the abundance of Si29 in presolar grains-Reference-Cited by-同舟云学术

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Spectroscopy of P30 and the abundance of Si29 in presolar grains

Published:2020-09-22 Issue:3 Volume:102 Page:
ISSN:2469-9985
Container-title:Physical Review C
language:en
Short-container-title:Phys. Rev. C

Author:

Lotay G.,Doherty D. T.,Seweryniak D.,Carpenter M. P.,Janssens R. V. F.^ORCID,José J.^ORCID,Rogers A. M.^ORCID,Woods P. J.,Zhu S.^ORCID

Funder

U.S. Department of Energy

Office of Science

Nuclear Physics

Ministerio de Economía, Industria y Competitividad, Gobierno de España

Federación Española de Enfermedades Raras

Agència de Gestió d’Ajuts Universitaris i de Recerca

Generalitat de Catalunya

European Cooperation in Science and Technology

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.102.035804/fulltext

Reference28 articles.

1. The Thermonuclear Runaway and the Classical Nova Outburst

2. NUCLEAR THERMOMETERS FOR CLASSICAL NOVAE

3. NUCLEAR MIXING METERS FOR CLASSICAL NOVAE

4. Nucleosynthesis in Classical Novae: CO versus ONe White Dwarfs

5. Nucleosynthesis in classical novae

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Nuclear Data Sheets for A=30;Nuclear Data Sheets;2024-10

2. Thermonuclear reaction rate of Si29(p,γ)P30;Physical Review C;2022-05-13

3. Hydrogen Burning of ²⁹Si and Its Impact on Presolar Stardust Grains from Classical Novae;The Astrophysical Journal;2022-04-01

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