One-dimensional Turbulence Models of Type I X-ray Bursts

One-dimensional Turbulence Models of Type I X-ray Bursts [electronic resource]

Type I X-ray bursts are caused by thermonuclear explosions occurring on the surface of an accreting neutron star in a binary star system. Observations and simulations of these phenomena are of great importance for understanding the fundamental properties of neutron stars and dense matter because the...

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Bibliographic Details
Online Access: Online Access (via OSTI)
Format: Government Document Electronic eBook
Language:English
Published: Washington, D.C. : Oak Ridge, Tenn. : United States. Department of Energy. Office of Nuclear Physics ; distributed by the Office of Scientific and Technical Information, U.S. Department of Energy, 2016.
Subjects:
Cosmic X-Ray Bursts.
Equations Of State.
Advection.
Neutron Stars.
Comparative Evaluations.
One-Dimensional Calculations.
Turbulence.
Carbon 12.
Thermonuclear Explosions.
Binary Stars.
Carbon Burning.
Stochastic Processes.
Abundance.
Expansion.
Mathematical Models.
Astronomy And Astrophysics.

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Call Number: E 1.99:doe-minnesota--sc0005012
E 1.99:doe-minnesota--sc0005012 Available

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