2003/02/11 by Avery E. Broderick, Avery Broderick, R. D. Blandford +1 · 6 citations
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Classical mechanics #Covariant transformation #Mathematical physics #Physics #Pulsars and Gravitational Waves Research #Theoretical physics #astro-ph
paper · pdf · doi:10.1046/j.1365-8711.2003.06618.x
published as Mon.Not.Roy.Astron.Soc. 342 (2003) 1280 · Submitted to MNRAS
arxiv created 2003/02/11 · openalex publication_date 2003/07/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
A considerable amount of effort has been invested in attempting to reproduce the spectral properties of accreting compact objects. A great deal of this work has been concerned with fitting the unpolarised flux with an underlying,