| Name | 085322 |
| Title | Monitoring the Extraordinary Timing Behavior of CCO Pulsars |
| URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853220201 |
| DOI | https://doi.org/10.57780/esa-qw0qrfj |
| Author | European Space Agency |
| Description | CCO pulsars are stable rotators with weak dipole B-fields and small spin-down rates, and are only detected in X-rays. We have been timing two CCO pulsars for 20 years. Surprisingly, we detected a glitch in the CCO 1E 1207.4-5209, which is unprecedented for any pulsar with such a small spin-down rate. This has profound implications for both the B-field evolution of CCOs and the mechanisms that trigger glitches. We are starting to see similar features in the timing of the CCO PSR J0821-4300 in Puppis A, and propose here to continue timing it to distinguish between glitch activity and an alternative of accretion torque noise at a very low level from fall-back disks around CCOs. |
| Publication | No observations found associated with the current proposal |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2019-10-09T03:22:12Z/2019-12-26T14:53:06Z |
| Version | 18.00_20191217_1110 |
| Mission Description | The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis. |
| Creator Contact | https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk |
| Date Published | 2021-01-14T23:00:00Z |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 2021, Monitoring The Extraordinary Timing Behavior Of Cco Pulsars, 18.00_20191217_1110, European Space Agency, https://doi.org/10.57780/esa-qw0qrfj |