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Shell-Flashes on Accreting Neutron Stars and Mode Profiles of Type-I X-Ray Bursts

Published online by Cambridge University Press:  14 August 2015

Shigeki Miyaji ,
Masayuki Y. Fujimoto  and
Tomoyuki Hanawa
Shigeki Miyaji
Affiliation:
Department of Earth Science and Astronomy, College of General Education, University of Tokyo
Masayuki Y. Fujimoto
Affiliation:
Department of Astronomy, University of Illinois
Tomoyuki Hanawa
Affiliation:
Department of Astronomy, University of Tokyo

Extract

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Thermal stabilities of hydrogen and helium shell-burnings on accreting neutron stars are studied semi-analytically, the progress of nuclear reactions during the flash is followed numerically, and the mechanism which makes different modes of Type-I X-ray bursts is discussed.

Type
Session 5: Mass-Accretion onto Compact Stars and Resultant Explosive Phenomena and Nucleosynthesis
Information
Symposium - International Astronomical Union , Volume 93: Fundamental Problems in the Theory of Stellar Evolution , 1981 , pp. 229 - 230
Copyright
Copyright © Reidel 1981