2000/01/07 by P. A. Caraveo, Caraveo, P. A.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Pulsars and Gravitational Waves Research #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0001112
LaTeX, 6 pages, 1 Postscript figure. Uses newpasp.sty. To appear in the Proceedings of IAU Colloquium 177 : "Pulsar Astronomy - 2000 & Beyond", Ed. Kramer, Wex & Wielebinski, ASP Conf.Series
arxiv created 2000/01/07 · openalex publication_date 2000/01/07 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Although less than 1% of all radio pulsars are detected at optical wavelengths, their optical emission can yield a wealth of information that is either very difficult or plainly impossible to obtain at other wavelengths.