CAPÍTULO 3. SOBRE LA EDUCACIÓN Y LOS PROCESOS EDUCATIVOS
3.3 Primeras reflexiones: Apuestas sobre la educación de las agrupaciones de músicas comunitarias
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The observed PSR sample is heavily biased. It is necessary to model the process of detection, i.e. to model the same surveys in the
synthetic Galaxy.
A synthetic PSR is detected if it appears in the area covered by on pf the survey, and if its radio flux exceeds some limit.
2/3 of known PSRs were detected in PBMPS or/and SM (914 and 151).
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To build an artificial model of a population of some astrophysical sources and to compare the results of calculations with observations.
Task:
Gould Belt : 20 NS Myr-1
Gal. Disk (3kpc) : 250 NS Myr-1
Arzoumanianet al.2002 ROSAT bCooling curves by bBlaschke et al. bMass spectrum 18° Gould Belt Gould Belt
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Mass spectrum of local young NSs can be different from the general one (in the Galaxy)
Hipparcos data on near-by massive stars
Progenitor vs NS mass: Timmes et al. (1996); Woosley et al. (2002)
Woosley et al. 2002