A dataset provided by the European Space Agency

Name 090234
Title Is PSR J1320-5359 heated by magnetic field decay?
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902340101

DOI https://doi.org/10.57780/esa-ci2dzdf
Author European Space Agency
Description Pulsar J1320-5359 was recently discovered to have one of the highest ever
measured long-term braking indices (n> 100). This is far in excess over the
canonical value of 3 that one would expect if pulsars slow down their rotation
as rotating magnetic dipoles. Although some variation of n (on the order of a
few) around 3 has been seen before, such extremely large braking indices are a
novel finding, and their physical origin is unclear. A promising hypothesis
suggests magnetic field decay as explanation. This can be observationally
checked since magnetic field decay should also manifest itself in an unusually
high thermal X-ray luminosity. Based on several properties, PSR J1320-5359 is
the best target to test whether the magnetic field decay hypothesis can explain the high braking indices.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-08-13T03:34:57Z/2022-08-13T18:18:17Z
Version 20.08_20220509_1852
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 2023-08-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, Is Psr J1320-5359 Heated By Magnetic Field Decayquestionmark, 20.08_20220509_1852, European Space Agency, https://doi.org/10.57780/esa-ci2dzdf