Pulse shape and spectrum of PSR J0218+4232 observed with BeppoSAX
| dc.creator | Mineo, T. | |
| dc.creator | Cusumano, G. | |
| dc.creator | Kuiper, L. | |
| dc.creator | Hermsen, W. | |
| dc.creator | Massaro, E. | |
| dc.creator | Becker, W. | |
| dc.creator | Nicastro, L. | |
| dc.creator | Sacco, B. | |
| dc.creator | Verbunt, F. | |
| dc.creator | Lyne, A. G. | |
| dc.creator | Stairs, I. H. | |
| dc.creator | Shibata, S. | |
| dc.date | 2000-01-20 | |
| dc.date.accessioned | 2026-07-07T01:51:49Z | |
| dc.date.available | 2026-07-07T01:51:49Z | |
| dc.description | We present the results of a BeppoSAX observation of PSR J0218+4232 which, for the first time, provides detailed information on the pulsar's temporal and spectral emission properties in the broad band 1-10 keV. We detected X-ray pulses with a pulsed fraction of 73 +/- 12 %. The pulse profile is characterized by two peaks phase separated by 0.47 +/-0.05. The pulsed spectrum is best described by a power-law of photon index 0.61 +/- 0.32 with an unabsorbed (2-10 keV) X-ray flux of 4.1E-13 erg/cm^2/s implying a luminosity of Lx = 1.3E32 Theta (d/5.7 kpc})^2 erg/s and an X-ray efficiency of 4.8E-4 Theta (d/5.7 kpc})^2 where Theta is the solid angle spanned by the emission beam. | |
| dc.description | 8 pages, 6 figures, accepted for publication on A&A | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0001355 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0001355 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/420 | |
| dc.subject | Astrophysics | |
| dc.title | Pulse shape and spectrum of PSR J0218+4232 observed with BeppoSAX | |
| dc.type | text |