A dataset provided by the European Space Agency

Name 072003
Title Probing the Binary Evolution of the ''Transition.. Object PSR J1023+0038


DOI https://doi.org/10.5270/esa-pig4px5
Author Dr Slavko Bogdanov
Description The binary radio millisecond pulsar PSR J1023+0038 appears to be a long sought- after ..missing link. between low-mass X-ray binaries and rotation-powered millisecond pulsars. We propose a deep spectroscopic and timing study of this system to look for any signature of recent accretion in this system in the pulsed thermal emission from the neutron star. This may offer unique insight into the little understood transition mechanism of millisecond pulsars from accretion power to rotation power.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-11-10T15:42:34Z/2013-11-12T06:04:14Z
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 2014-11-26T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-11-26T00:00:00Z, 072003, 17.56_20190403_1200. https://doi.org/10.5270/esa-pig4px5