1998/03/03 by V. M. Kaspi, Kaspi, V. M.
Computer Science · Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Geophysics and Gravity Measurements #Pulsars and Gravitational Waves Research #Seismology and Earthquake Studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9803026
8 pages Postscript. To appear in Proceedings of the Symposium "Neutron Stars and Pulsars", held in Tokyo, Japan, November 17-20, 1997. Universal Academy Press, in press
arxiv created 1998/03/03 · openalex publication_date 1998/03/03 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We summarize the current observational evidence for associations between supernova remnants and neutron stars, including radio pulsars, proposed "inactive" young neutron stars, "anomalous" X-ray pulsars, and soft gamma-ray repeaters, and argue that the paradigm that all young neutron stars are Crab-like requires reconsideration.