PSR J1738+0333: a new gravitational laboratory
| dc.creator | Freire, Paulo C. C. | |
| dc.creator | Jacoby, Bryan A. | |
| dc.creator | Bailes, Matthew | |
| dc.date | 2007-11-12 | |
| dc.date.accessioned | 2026-07-07T11:13:07Z | |
| dc.date.available | 2026-07-07T11:13:07Z | |
| dc.description | We describe in this paper a new binary millisecond pulsar, PSR J1738+0333. Using Arecibo, we have achieved good timing accuracy for this object, about 220 ns for 1-hour integrations over 100 MHz. This allowed us to measure a precise proper motion, parallax and orbital parameters for this system. We highlight the system's potential for constraining alternative theories of gravitation. | |
| dc.description | 3 pages, 2 figures. To appear in the proceedings of "40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More", August 12-17, 2007, McGill University, Montreal, Canada | |
| dc.identifier | https://arxiv.org/abs/0711.1880 | |
| dc.identifier | http://arxiv.org/abs/0711.1880 | |
| dc.identifier | AIPConf.Proc.983:488-490,2008 | |
| dc.identifier | doi:10.1063/1.2900281 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/191607 | |
| dc.subject | Astrophysics | |
| dc.title | PSR J1738+0333: a new gravitational laboratory | |
| dc.type | text |