|Title||PSR B1929+10 - the most serious challenge for electron acceleration in a PWN|
|Author||Prof Werner Becker|
|Description||XMM-Newton has confirmed the existence of the diffuse X-ray emission with a trail morphology lying in a direction opposite to the transverse motion of the million year old pulsar PSR B1929+10. A possible interpretation of the emission is that it is a synchrotron wake from particles left behind by the pulsar as it moves through the ISM. We propose deep spectro-imaging observations of the pulsar.s X-ray trail with XMM-Newton in order to explore the emission processes at work and to measure its length-width and spectral evolution as a function of distance from the pulsar.|
|Publication||The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
A deep X-ray spectral imaging of the bow-shock pulsar wind nebula associated with PSR B1929+10 . Kim, S. I., Hui, C. Y., et all. . A&A . 637-7 . 2020 . 2020A&A...637L...7K ,
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2014-04-27T00:00:00Z, 069520, 17.56_20190403_1200. https://doi.org/10.5270/esa-q22wghq|