A dataset provided by the European Space Agency

Name 055067
Title Measuring the Magnetic Fields of Central Compact Objects in Supernova Remnants
URL

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DOI 10.5270/esa-hwfpuuv
Author Prof Jules Halpern
Description X-ray timing studies of two X-ray pulsars in SNRs have detected no braking of their rotation, implying upper limits of 3E11 G on their surface dipole fields, well below those of ordinary young pulsars. We proposed that weak B-fields related to slow natal spin may be the physical basis of the class of Central Compact Objects (CCOs), including the unseen pulsar in SN 1987A. This proposal leverages existing timing data on CCO pulsars to determine if they are spinning down and, if so, to measure their magnetic fields by obtaining coherent timing solutions linking all previous data. Fields as small as 1E10 G can be measured in this way. Alternatively, accretion of supernova debris through a fallback disk may be occurring, which would be detectable as torque noise.
Publication Spin-Down Measurement of PSR J1852+0040 in Kesteven 79: Central Compact Objects as Anti-Magnetars . Halpern, J. P., Gotthelf, E. V., . ApJ . 709-436 . 2010 . 2010ApJ...709..436H ,
Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution models . Vigano, D., Rea, N., et all. . MNRAS . 434-123 . 2013 . 2013MNRAS.434..123V ,
Discovery of the Transient Magnetar 3XMM J185246.6+003317 near Supernova Remnant Kesteven 79 with XMM-Newton . Zhou, Ping, Chen, Yang, et all. . ApJ . 781-16 . 2014 . 2014ApJ...781L..16Z ,
3XMM J185246.6+003317: Another Low Magnetic Field Magnetar . Rea, N., Vigano, D., et all. . ApJ . 781-17 . 2014 . 2014ApJ...781L..17R ,
Fermi-LAT Observations of Supernova Remnants Kesteven 79 . Auchettl, Katie, Slane, Patrick, . ApJ . 783-32 . 2014 . 2014ApJ...783...32A ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
3XMM J185246.6+003317 as transient neutron star . Hambaryan, V., Wagner, D., et all. . AN . 336-545 . 2015 . 2015AN....336..545H ,
Modeling the X-Rays from the Central Compact Object PSR J1852+0040 in Kesteven 79: Evidence for a Strongly Magnetized Neutron Star . Bogdanov, Slavko, . ApJ . 790-94 . 2014 . 2014ApJ...790...94B ,
The Million Opt...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-09-19T16:41:23Z/2009-04-23T05:22:27Z
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 2010-05-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-05-20T00:00:00Z, 055067, 17.56_20190403_1200. https://doi.org/10.5270/esa-hwfpuuv