M. Coleman Miller

TL;DR: The history and advancements of gravitational-wave astronomy are reviewed, the future of the field is discussed, and a focus on multi-messenger astronomy is led.

TL;DR: In this article, the authors make general relativistic calculations of the light curves and oscillation amplitudes produced by a rotating neutron star with one or two hot spots as a function of spot size, stellar compactness, rotational velocity at the stellar surface, spot location, orientation of the line of sight of the observer, and angular dependence of the surface specific intensity.

TL;DR: In this article, it was shown that a reasonable quantitative agreement with data requires that the characteristic radius of the tidal stream is approximately equal to the semimajor axis of the most bound orbit of the debris rather than twice the pericenter distance.

TL;DR: The enhanced X-ray Timing and Polarimetry (eXTP) mission as discussed by the authors was proposed for studies related to Observatory Science targets, such as flaring stars, supernova remnants, accreting white dwarfs, low and high mass Xray binaries, radio quiet and radio loud active galactic nuclei, tidal disruption events, and gamma-ray bursts.

TL;DR: In this article, the authors consider the total power requirements and show that the only viable power source associated with isolated neutron stars is rotation, and demonstrate that not enough rotational energy is tapped by a propeller II-like acceleration of interstellar matter.