A Sociological Study of the Optically Emitting Isolated Neutron Stars

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dc.creatorCaraveo, P. A.
dc.date2000-01-07
dc.date.accessioned2026-07-07T01:51:36Z
dc.date.available2026-07-07T01:51:36Z
dc.descriptionAlthough 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.
dc.descriptionLaTeX, 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0001112
dc.identifierhttp://arxiv.org/abs/astro-ph/0001112
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/350
dc.subjectAstrophysics
dc.titleA Sociological Study of the Optically Emitting Isolated Neutron Stars
dc.typetext

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