2002/11/30 by Chris Done, C. Done, Marek Gierlinski +1 · 7 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #Event (particle physics) #Event horizon #Horizon #Neutron star #Pulsars and Gravitational Waves Research #Stars #Stellar black hole #astro-ph
paper · pdf · doi:10.1046/j.1365-8711.2003.06614.x
published as Mon.Not.Roy.Astron.Soc.342:1041,2003 · 13 pages, 12 figures, accepted for publication in MNRAS
arxiv created 2003/04/01 · openalex publication_date 2003/07/11 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The key difference between neutron stars and black holes is the presence/absence of a solid surface. Recent attempts to detect this difference have concentrated on the quiescent luminosity, but here these sources are faint and difficult to observe. Instead we look at these sources when they are bright, and show that there is a clear difference between black holes and neutron stars in the evolution of their X-ray spectra, which is due to the presence of a surface in the case of neutron stars. We also show that there is a type of X-ray spectrum that is only seen from black holes, making it a good diagnostic for the nature of new transient sources.