Thermonuclear model for x-ray transients

Thermonuclear model for x-ray transients [electronic resource]

The thermonuclear evolution of a 1.41 M sub solar neutron star accreting both solar and metal-deficient mixtures of hydrogen, helium, and heavy elements at rates ranging from about 10/sup -11/ to 10/sup -10/ M sub solar per year is examined using a one-dimensional numerical model. The metal deficien...

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Bibliographic Details
Online Access: Online Access
Corporate Author: Los Alamos National Laboratory (Researcher)
Format: Government Document Electronic eBook
Language:English
Published: Los Alamos, N.M. : Oak Ridge, Tenn. : Los Alamos National Laboratory ; distributed by the Office of Scientific and Technical Information, U.S. Department of Energy, 1982.
Subjects:
Neutron Stars.
Star Accretion.
Cosmic Gamma Bursts.
Helium Burning.
Hydrogen Burning.
Numerical Solution.
One-Dimensional Calculations.
Star Models.
Cosmic Radiation.
Ionizing Radiations.
Mathematical Models.
Primary Cosmic Radiation.
Radiations.
Star Burning.
Star Evolution.
Stars.
Classical And Quantum Mechanics, General Physics.

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Call Number: E 1.99:la-ur-82-1396
E 1.99:la-ur-82-1396 Available

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