The reactions and ashes of thermonuclear explosions on neutron stars

被引：13

作者：

Fisker, JL ^{[1
]}

Brown, EF

Liebendörfer, M

Thielemann, FK

Wiescher, M

机构：

[1] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA

[2] Univ Notre Dame, Joint Inst Nucl Astrophys, Notre Dame, IN 46556 USA

[3] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA

[4] Michigan State Univ, Joint Inst Nucl Astrophys, E Lansing, MI 48824 USA

[5] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada

[6] Dept Phys & Astron, CH-4056 Basel, Switzerland

来源：

NUCLEAR PHYSICS A | 2005年 / 752卷

关键词：

D O I：

10.1016/j.nuclphysa.2005.02.063

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

This paper reports on the detailed rp-process reaction flow on an accreting neutron star and the resulting ashes of a type 1 X-ray burst. It is obtained by coupling a 298 isotope reaction network to a self-consistent one-dimensional model calculation with a constant accretion rate of M = 10(17) g/s.

引用

页码：604C / 607C

页数：4

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