activity
19942026
most citedFormation of Double Neutron Star Systems

698 citations · 3.2k across the 85 of their papers we have counts for

collaborators
Showing 2010Show all

7 papers · 1 filter

astro-ph.SR2010★ 25 cited

Revisiting the Flowers-Ruderman instability of magnetic stars

Pablo Marchant, Andreas Reisenegger, Taner Akgün

In 1977, Flowers and Ruderman described a perturbation that destabilises a purely dipolar magnetic field in a fluid star. They considered the effect of cutting the star in half alo…

astro-ph.HE2010★ 9 cited

Long-period thermal oscillations in superfluid millisecond pulsars

Cristobal Petrovich, Andreas Reisenegger

In previous papers, we have shown that, as the rotation of a neutron star slows down, it will be internally heated as a consequence of the progressively changing mix of particles (…

astro-ph.HE2010★ 100 cited

Internal Heating of Old Neutron Stars: Contrasting Different Mechanisms

Denis Gonzalez, Andreas Reisenegger

Context: The standard cooling models of neutron stars predict temperatures K for ages yr. However, the likely thermal emission detected from the millisecond p…

astro-ph.HE2010

Rotochemical heating with a density-dependent superfluid energy gap in neutron stars

Nicolás González-Jiménez, Cristóbal Petrovich, Andreas Reisenegger

When a rotating neutron star loses angular momentum, the reduction of the centrifugal force makes it contract. This perturbs each fluid element, raising the local pressure and orig…

astro-ph.SR2010★ 30 cited

Asymptotic, non-linear solutions for ambipolar diffusion in one dimension

Jaime Hoyos, Andreas Reisenegger, Juan Valdivia

We study the effect of the non-linear process of ambipolar diffusion (joint transport of magnetic flux and charged particles relative to neutral particles) on the long-term behavio…

astro-ph.HE2010★ 8 cited

Internal Heating of Old Neutron Stars: Contrasting Different Mechanisms

Denis Gonzalez, Andreas Reisenegger, Rodrigo Fernandez

The thermal emission detected from the millisecond pulsar J0437-4715 is not explained by standard cooling models of neutron stars without a heating mechanism. We investigated three…