A dataset provided by the European Space Agency

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
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803620301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803620401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803620501

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