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Persistent and transient blank field sources

2006/09/07 by A. Treves, S. Campana, M. Chieregato +3 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Blank #Cosmology #Field (mathematics) #Neutron star #Pulsars and Gravitational Waves Research #ROSAT #Transient (computer programming) #astro-ph

paper · pdf · doi:10.1007/s10509-007-9346-6

published as Astrophys.SpaceSci.308:167-169,2007 · 3 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

arxiv created 2006/09/07 · openalex publication_date 2007/03/23 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Blank 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.

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