ROSAT archival observations of 1SAX J0054.9-7226 = 2E 0053.2-7242, a newly discovered X-ray pulsar in the SMC
| dc.creator | Israel, G. L. | |
| dc.creator | Campana, S. | |
| dc.creator | Cusumano, G. | |
| dc.creator | Frontera, F. | |
| dc.creator | Orlandini, M. | |
| dc.creator | Santangelo, A. | |
| dc.creator | Stella, L. | |
| dc.date | 1998-04-20 | |
| dc.date.accessioned | 2026-07-07T02:26:38Z | |
| dc.date.available | 2026-07-07T02:26:38Z | |
| dc.description | We analysed 13 archival ROSAT PSPC and HRI observations which included the position of a newly discovered 59s X-ray pulsar in the Small Magellanic Cloud, 1SAX J0054.9-7226 = 2E 0053.2-7242. The source was detected three times between 1991 and 1996 at a luminosity level ranging from about 8 x 10^{34} - 4 x 10^{35} erg s^{-1} (0.1-2.4 keV). Highly significant pulsations at 59.072s were detected during the 1991 October 8-9 observation. The ROSAT period, together with those measured by RXTE and BeppoSAX yields a period derivative of Pdot = - 0.016 s yr^{-1}. A much more accurate source position (10 arcsec uncertainty) was obtained through the ROSAT HRI detection on 1996 April restricting to three m_V > 15.5 stars the likely counterpart of 1SAX J0054.9-7226 = 2E 0053.2-7242. | |
| dc.description | 4 pages (figures included). Accepted for publication on A&A Letters | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9804186 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9804186 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12351 | |
| dc.subject | Astrophysics | |
| dc.title | ROSAT archival observations of 1SAX J0054.9-7226 = 2E 0053.2-7242, a newly discovered X-ray pulsar in the SMC | |
| dc.type | text |