Once formed, they no longer actively generate heat, and cool over time; however, they may still evolve further through collision or accretion. Most of the basic models for these objects imply that ...

Using the X-ray Polarimetry Explorer (IXPE) and Neutron star Interior Composition Explorer (NICER), Indian astronomers have ...

A Los Alamos simulation of an accretion disk after the collision of two neutron stars. This event generates both light (blue) and heavy (red) elements. Disclaimer: AAAS and EurekAlert! are not ...

They are believed to be powered by the accretion of material onto black holes or neutron stars, and their study has gained significant momentum in recent years. Researchers are particularly ...

Publications of the Astronomical Society of the Pacific, Vol. 118, No. 846 (August 2006), pp. 1098-1103 (6 pages) ABSTRACT It has been argued that there is a linear correlation between star formation ...

Was a powerful cosmic explosion seen by the Einstein Probe launched by a supermassive black hole snacking on a star, by a ...

[Image description: In the foreground, at the centre right, there is a very bright white ball, representing the neutron star. White/purple filaments are streaming out from its polar region.

Be stars also show excess in Infrared (IR) emission. X-Ray Pulsars are magnetized Neutron Stars. In Binary systems, when the Neutron Star enters the accretion regime, it starts to accrete matter from ...

Interacting binary stars are systems where two stars are in close proximity, allowing them to exchange mass and energy. This interaction often leads to the formation of accretion disks, which are ...

These sources, known as ultra-luminous X-ray pulsars (ULXPs), are neutron stars typically less massive ... suggesting the change in accretion dynamics with mass accretion rate.

Li, '23, "Properties of Slicing Conditions for Charged Black Holes" Sophia Schnauck, '22, "Accretion Onto a Black Hole at the Center of a Neutron Star: Nuclear Equations of State" Kieran Enzian, '22, ...