Discovery of a faint 437 s X-ray pulsar 1SAX J1452.8-5949
| dc.creator | Oosterbroek, T. | |
| dc.creator | Orlandini, M. | |
| dc.creator | Parmar, A. N. | |
| dc.creator | Angelini, L. | |
| dc.creator | Israel, G. L. | |
| dc.creator | Fiume, D. Dal | |
| dc.creator | Mereghetti, S. | |
| dc.creator | Santangelo, A. | |
| dc.creator | Cusumano, G. | |
| dc.date | 1999-10-21 | |
| dc.date.accessioned | 2026-07-07T02:33:58Z | |
| dc.date.available | 2026-07-07T02:33:58Z | |
| dc.description | A new pulsar, 1SAX J1452.8-5949, was discovered during a BeppoSAX galactic plane survey on 1999 July 20 at R.A.=14h 52m 49s, Dec=-59 49' 18'' (J2000) with a 90% confidence uncertainty radius of 50''. Coherent pulsations were detected with a barycentric period of a 437.4 +/- 1.4 s. The X-ray spectrum can be modeled by a power-law with a photon index of 1.4 +/- 0.6 and absorption consistent with the galactic value in the direction of the source ($1.9 \times 10^{22}$ atom cm$^{-2}$). An Fe K line with a equivalent width of $\approxgt$1.3 keV may be present in the spectrum. The unabsorbed 2-10 keV flux is $9 \times 10^{-13}$ erg cm$^{-2}$s$^{-1}$. The X-ray properties and lack of an obvious optical counterpart are consistent with a Be star companion at a distance of between approximately 6 and 12 kpc which implies a luminosity of (4-15)$\times 10^{33}$ erg s$^{-1}$. | |
| dc.description | Accepted for publication in Astronomy and Astrophysics Letters | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9910384 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9910384 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15061 | |
| dc.subject | Astrophysics | |
| dc.title | Discovery of a faint 437 s X-ray pulsar 1SAX J1452.8-5949 | |
| dc.type | text |