A dataset provided by the European Space Agency

Name 078333
Title Unraveling the cause of intermittent accretion in PSRJ1023+0038 with XMM and VLT
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783330301

DOI 10.5270/esa-cwy5f9p
Author Dr Cees Bassa
Description The binary millisecond pulsar J1023+0038 is one of only three sources that have been observed to transition between a radio millisecond pulsar and a low-mass X-ray binary state. In the low-mass X-ray binary state, the system exhibits discrete high and low modes in X-ray flux, between which it rapidly switches on minute-long timescales. Coherent X-ray pulsations at the spin period of the neutron star are observed only during the high X-ray flux modes. For the first time, we are seeing coherent X-ray pulsations from a neutron star accreting at very low luminosity (10e33 erg-s). The rapid on-off switching of the
Publication Timing Observations of PSR J1023+0038 During a Low-mass X-Ray Binary State . Jaodand, Amruta, Archibald, Anne M., et all. . ApJ . 830-122 . 2016 . 2016ApJ...830..122J ,
Simultaneous broadband observations and high-resolution X-ray spectroscopy of the transitional millisecond pulsar PSR J1023+0038 . Coti Zelati, F., Campana, S., et all. . A&A . 611-14 . 2018 . 2018A&A...611A..14C ,
The First Continuous Optical Monitoring of the Transitional Millisecond Pulsar PSR J1023+0038 with Kepler . Papitto, A., Rea, N., et all. . ApJ . 858-12 . 2018 . 2018ApJ...858L..12P ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2015-12-09T00:46:19Z/2015-12-09T08:27:59Z
Version 17.56_20190403_1200
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 2017-01-07T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017-01-07T23:00:00Z, 078333, 17.56_20190403_1200. https://doi.org/10.5270/esa-cwy5f9p