M. Coleman Miller

TL;DR: In this paper, the mass and radius estimates of rotation-powered millisecond pulsars were analyzed using the X-ray pulse profile models used to obtain information about the mass-radius relation of neutron stars and the equation of state of dense matter in their cores.

TL;DR: In this paper, the authors investigate the ability of a future UHE neutrino detector to identify the brightest neutrinos point sources, by exploring the parameter space of the total number of observed events and the angular resolution of the detector.

TL;DR: In this paper, the authors use a point-likelihood technique to show that the observed period clustering is not simply a statistical fluctuation, and quantify the constraints it imposes on the birth period and on the final period of such systems.

TL;DR: A review of the current major challenges in stellar cluster research can be found in this paper, including young clusters, globular clusters, and galactic nuclei, including primordial mass segregation and runaway mergers, expulsion of gas from clusters, production of stellar exotica seen in some clusters, binary populations within clusters, the black-hole population within stellar clusters, stellar dynamics around a massive black hole, and stellar collisions.

TL;DR: In this paper, the authors report the recent advances in Relativistic Astrophysics as presented at the GR20 meeting in Warsaw, Poland, in July 2013, and present a survey of these advances.