Persistent and Transient Blank Field Sources

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dc.creatorTreves, A.
dc.creatorCampana, S.
dc.creatorChieregato, M.
dc.creatorMoretti, A.
dc.creatorNelson, T.
dc.creatorOrio, M.
dc.date2006-09-07
dc.date.accessioned2026-07-07T10:40:04Z
dc.date.available2026-07-07T10:40:04Z
dc.descriptionBlank field sources (BFS) are good candidates for hosting dim isolated neutron stars (DINS). The results of a search of BFS in the ROSAT HRI images are revised. We then focus on transient BFS, arguing that they belong to a rather large population. The perspectives of future research on DINS are then discussed.
dc.description3 pages, 0 figures. Paper presented at the Conference "Isolated Neutron Stars: from the interior to the surface", London, April 2006. Astrophysics and Space Science, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0609194
dc.identifierhttp://arxiv.org/abs/astro-ph/0609194
dc.identifierAstrophys.SpaceSci.308:167-169,2007
dc.identifierdoi:10.1007/s10509-007-9346-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181239
dc.subjectAstrophysics
dc.titlePersistent and Transient Blank Field Sources
dc.typetext

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