New insights from a global view of X-ray bursts

It is shown here that the behavior of nuclear burning on accreting neutron stars depends on the mass accretion rate per unit area sigma-dot, the temperature T, and the column density of accreted matter sigma, and is thus intrinsically a three-dimensional problem. The concepts of a nuclear fuel surfa...

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Bibliographische Detailangaben
Veröffentlicht in:	Astrophys. J.; (United States) 1987-12, Vol.323 (1), p.55-60
Hauptverfasser:	Fushiki, Ikko, Lamb, D. Q.
Format:	Artikel
Sprache:	eng
Schlagworte:	640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources Astronomy Astrophysics CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC RAY SOURCES COSMIC X-RAY BURSTS COSMIC X-RAY SOURCES Earth, ocean, space ENERGY SOURCES Exact sciences and technology FUELS Late stages of stellar evolution (including black holes) MATERIALS MATHEMATICAL MODELS NEUTRON STARS NUCLEAR FUELS NUCLEAR REACTIONS REACTOR MATERIALS STAR ACCRETION STAR EVOLUTION STARS TEMPERATURE DEPENDENCE
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