Name | 080362 |
Title | Continued Timing of PSR J1023+0038: A Unique Testbed for Accretion Physics |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803620201 |
DOI | https://doi.org/10.5270/esa-y3zlu2f |
Author | European Space Agency |
Description | Three years ago, PSR J1023+0038 (J1023) transformed from a rotation-powered millisecond pulsar state to an accretion-disk-dominated X-ray pulsar state. In this state it shows coherent X-ray pulsations indicating active accretion at low luminosities. Using these pulsations we have discovered that in the X-ray state J1023 is spinning down 27% faster than the radio state (Jaodand et al. 2016). Along with this unique, long-term X-ray timing solution for a transitional millisecond pulsar (tMSP) we also find a change in average orbital period derivative between states. Extending the span of our timing solution to a possible J1023 transition (back to radio) in the coming year(s) is critical to understand tMSP transitions and accretion physics. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2017-05-08T21:33:24Z/2017-06-13T20:19:02Z |
Version | 19.17_20220121_1250 |
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 | 2018-07-03T22:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2018, Continued Timing Of Psr J1023+0038: A Unique Testbed For Accretion Physics, 19.17_20220121_1250, European Space Agency, https://doi.org/10.5270/esa-y3zlu2f |