M. Coleman Miller

TL;DR: In this paper, the authors proposed a model for the X-ray emission from 14 neutron stars in low-mass binary systems and from another neutron star in the direction of the Galactic center.

TL;DR: In this paper, the authors explore a model for these sources and suggest that in some tens of per cent of globular clusters a very massive black hole, M≳50 m⊙, is formed.

TL;DR: In the last few years, it was generally believed that black holes in nature appear in two broad mass ranges: stellar-mass (M ∼ 3 − 20 M⊙) which are produced by the core collapse of massive stars, and supermassive (m ∼ 10 6 − 10 10 10 M ⊙), which are found in the centers of galaxies and are generated by a still uncertain combination of processes as mentioned in this paper.

TL;DR: In this paper, a review of the current state of knowledge and an outline of some of the outstanding questions that still need to be addressed is provided, based on discussions at a workshop hosted by the Albert Einstein Institute in Golm, Germany.

TL;DR: In this article, the authors proposed three models of angular momentum transport in massive stars: a mildly efficient transport by meridional currents, an efficient transport implemented in the MESA code, and a very efficient transport to calculate natal BH spins.