|Title||Completing the X-ray census of Plerionic Supernova Remnants within 7 kpc|
|Author||Dr Oleg Kargaltsev|
|Description||Supernova Remnants of center-filled and composite types often host young, energetic pulsars emitting strong relativistic winds. Chandra and XMM-Newton observations of such SNRs have already resulted in a number of pulsar and pulsar-wind nebula (PWN) discoveries. We propose to complete the X-ray census of plerionic remnants within a 7 kpc distance, which we have begun in XMM-Newton AO-4. The SNRs were selected based on their radio morphologies and archival ROSAT or ASCA data. This short survey will substantially expand the sample of PNWe and pulsars observed in X-rays and help to establish the properties of the overall population.|
|Publication||No observations found associated with the current proposal|
|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, 2007-11-22T00:00:00Z, 040091, 17.56_20190403_1200. https://doi.org/10.5270/esa-w20i102|