A dataset provided by the European Space Agency

Name 072260
Title Measuring the Spin Period of a High-Velocity Pulsar
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722600101

DOI 10.5270/esa-n2gwqyn
Author Dr John Tomsick
Description X-ray observations of IGR J11014-6103 show that it has a complex morphology with a point source and two components of extended emission. Its properties indicate that it is very likely to be a pulsar wind nebula (PWN). Chandra and radio observations strongly suggest that the compact object is moving away from SNR MSH 11-61A. Based on the evolution of this supernova remnant, an association would indicate that IGR J11014-6103 has a transverse velocity of 2,400 to 2,900 km-s. The possibility of such a high kick velocity makes the proposed timing study important for proving that the compact object is a pulsar, determining its period (P), and measuring dP-dt to determine if the characteristic age is consistent with the pulsar originating in MSH 11-61A.
Publication Discovery of X-Ray Pulsations from the INTEGRAL Source IGR J11014-6103 . Halpern, J. P., Tomsick, J. A., et all. . ApJ . 795-27 . 2014 . 2014ApJ...795L..27H ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-07-21T00:24:04Z/2013-07-21T13:40:44Z
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 2014-08-31T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-08-31T00:00:00Z, 072260, 17.56_20190403_1200. https://doi.org/10.5270/esa-n2gwqyn