| Proposal ID | 065277 |
| Title | A dark twin of the Crab |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652770101 |
| DOI | https://doi.org/10.5270/esa-gxmhble |
| Principal Investigator, PI | Dr Oleg Kargaltsev |
| Abstract | We propose an EPIC observation of the recently discovered young PSR J2022+3842.Compared to other young pulsars in our Galaxy, J2022+3842 is exceptionallypowerful and has the shortest spin period. An archival Chandra image hasrevealed a point source and a faint compact nebula with puzzling X-rayproperties. The X-ray efficiencies of the pulsar and its PWN are orders ofmagnitude lower than one would expect for such a powerful pulsar. On the otherhand, the object is still bright enough to allow a detailed study in X-rays. Wewill carry out a joint phase-resolved, multiwavelength analysis to betterunderstand the radiatively-inefficient energy loss mechanism of this outstandingpulsar. We will also look for a large-scale X-ray emission from the PWN and the host SNR. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2011-04-14T08:01:25Z/2011-04-15T21:57:27Z |
| Version | 17.56_20190403_1200 |
| Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 | 2012-05-05T00:00:00Z |
| Keywords | "faint compact nebula", "xray properties", "phase resolved", "supernova remnant", "magnitude lower", "dark twin", "archival chandra image", "psr j2022", "xray efficiencies", "EPIC", "multiwavelength analysis", "scale xray emission", "shortest spin period" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Oleg Kargaltsev, 2012, 'A dark twin of the Crab', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gxmhble |