Amanote Research

Amanote Research

    RegisterSign In

Cooling of the Cassiopeia a Neutron Star and the Effect of Diffusive Nuclear Burning

doi 10.1063/1.5117797
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 2019

Authors
Wynn C. G. HoM. J. P. WijngaardenPhilip ChangCraig O. HeinkeDany PageMikhail BeznogovDaniel J. Patnaude
Publisher

AIP Publishing


Related search

Magnetic Neutron Star Cooling and Microphysics

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2018English

Thermonuclear Burning in the Envelope of an Accreting Neutron Star

Symposium - International Astronomical Union
1980English

The Effect of Rotation on the Stability of Nuclear Burning in Accreting Neutron Stars

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2009English

The Effects of Δ Meson on the Neutron Star Cooling

Plasma Science and Technology
Condensed Matter Physics
2012English

Neutron Star Properties and the Nuclear Equation of State

2012English

Neutron Star-Black Hole Mergers With a Nuclear Equation of State and Neutrino Cooling: Dependence in the Binary Parameters

Physical Review D
2014English

An Algorithm for the Simulation of the Magnetized Neutron Star Cooling

EPJ Web of Conferences
AstronomyPhysics
2016English

The Effect of the Diffusive-Thermal Instability on the Burning Velocity of Cellular Flames.

Journal of the Japan Society for Aeronautical and Space Sciences
1997English

The Inner Boundary of a Neutron-Star Crust

Nuclear Physics A
High Energy PhysicsNuclear
1995English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2026 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy