A dataset provided by the European Space Agency

Name 050204
Title Measuring the Spin-downs of Three Nearby Isolated Neutron Stars
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502040601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502040701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502040801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502040901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502041001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502041101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502041201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502041301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502041401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502041501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502041701
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502041801

DOI https://doi.org/10.5270/esa-xpfteuw
Author Dr David Kaplan
Description The nearest thermally emitting neutron stars may be the best sample to measure
the true demographics of neutron stars, and arguably offer the best prospects
for measuring neutron star radii through thermal emission. But these tasks are
complicated by our lack of knowledge about their magnetic field strengths and
ages. Recently, we have determined these for two objects using dedicated X-ray
timing observations: by measuring spin-down and assuming a dipole field, we find
magnetic fields between normal pulsars and magnetars. We propose to complete
this sample with timing observations of the three remaining objects in this
class that show periodicities: RX J0420.0-5022, RX J0806.4-4123, and RX
J2143.0+0654.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-05-13T16:27:08Z/2008-05-19T06:27:05Z
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 2009-06-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr David Kaplan, 2009, 050204, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xpfteuw