NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-04-20 T23:19:34 PDT
Help | Comment | NED Home

For refcode 2008MNRAS.384.1638P:
Retrieve 188 NED objects in this reference.
Please click here for ADS abstract

NED Abstract

Copyright by Royal Astronomical Society. 2008MNRAS.384.1638P How rapidly do neutron stars spin at birth? Constraints from archival X-ray observations of extragalactic supernovae Perna, Rosalba; Soria, Roberto; Pooley, Dave; Stella, Luigi Abstract. Traditionally, studies aimed at inferring the distribution of birth periods of neutron stars are based on radio surveys. Here we propose an independent method to constrain the pulsar spin periods at birth based on their X-ray luminosities. In particular, the observed luminosity distribution of supernovae (SNe) poses a constraint on the initial rotational energy of the embedded pulsars, via the correlation found for radio pulsars, and under the assumption that this relation continues to hold beyond the observed range. We have extracted X-ray luminosities (or limits) for a large sample of historical SNe observed with Chandra, XMM and Swift, which have been firmly classified as core-collapse SNe. We have then compared these observational limits with the results of Monte Carlo simulations of the pulsar X-ray luminosity distribution for a range of values of the birth parameters. We find that a pulsar population dominated by millisecond periods at birth is ruled out by the data. Key words: supernova remnants, pulsars: general, X-rays: stars
Retrieve 188 NED objects in this reference.
Please click here for ADS abstract

Back to NED Home