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- W3102087918 abstract "We present our new advanced model for population synthesis of close-by cooling NSs. Detailed treatment of the initial spatial distribution of NS progenitors and a detailed ISM structure up to 3 kpc give us an opportunity to discuss the strategy to look for new isolated cooling NSs. Our main results in this respect are the following: new candidates are expected to be identified behind the Gould Belt, in directions to rich OB associations, in particular in the Cygnus-Cepheus region; new candidates, on average, are expected to be hotter than the known population of cooling NS. Besides the usual approach (looking for soft X-ray sources), the search in 'empty' $gamma$-ray error boxes or among run-away OB stars may yield new X-ray thermally emitting NS candidates." @default.
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- W3102087918 date "2008-01-01" @default.
- W3102087918 modified "2023-09-27" @default.
- W3102087918 title "Space cowboys odyssey: beyond the Gould Belt" @default.
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- W3102087918 doi "https://doi.org/10.1063/1.2900196" @default.
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