Space cowboys odyssey: Beyond the Gould Belt

S. B. Popov, B. Posselt, F. Haberl, J. Trümper, R. Turolla, R. Neuhäuser

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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' γ-ray error boxes or among run-away OB stars may yield new X-ray thermally emitting NS candidates.

Original languageEnglish (US)
Title of host publication40 Years Of Pulsars
Subtitle of host publicationMillisecond Pulsars, Magnetars and More
Pages357-359
Number of pages3
DOIs
Publication statusPublished - Mar 20 2008
Event40 Years Of Pulsars: Millisecond Pulsars, Magnetars and More - Montreal, QC, Canada
Duration: Aug 12 2007Aug 17 2007

Publication series

NameAIP Conference Proceedings
Volume983
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

Other40 Years Of Pulsars: Millisecond Pulsars, Magnetars and More
CountryCanada
CityMontreal, QC
Period8/12/078/17/07

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All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Cite this

Popov, S. B., Posselt, B., Haberl, F., Trümper, J., Turolla, R., & Neuhäuser, R. (2008). Space cowboys odyssey: Beyond the Gould Belt. In 40 Years Of Pulsars: Millisecond Pulsars, Magnetars and More (pp. 357-359). (AIP Conference Proceedings; Vol. 983). https://doi.org/10.1063/1.2900196