| Proposal ID | 040662 |
| Title | Why are millisecond pulsar magnetic fields low and how do their X-rays arise |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0406620201 |
| DOI | https://doi.org/10.5270/esa-xgy81xz |
| Principal Investigator, PI | Dr Natalie Webb |
| Abstract | Binary millisecond pulsars (MSPs) found in the field are thought to berecycled from accreting pulsars. These MSPs have short periods, low spindownrates (Pdot) and consequently low surface magnetic fields (B_s) as B_s isproportional to sqrt(Pdot.P). It is unclear, however, how the MSP B_s can evolvefrom the high fields observed in pulsars to the low MSP values. Two models havebeen proposed to explain this evolution. Further, the origin of the high energyemission is unclear with too few MSP observations in the X-ray domain todifferentiate between competing models. With these XMM-Newton observations offour MSPs previously unobserved in X-rays, we will discriminate betweendiffering models describing the magnetic field evolution and the high energy emission origin. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2007-03-22T13:41:31Z/2007-04-28T07:26:29Z |
| 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 | 2008-09-27T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "magnetic field evolution", "differing models describing", "msp b_s", "short periods", "xmm newton", "accreting pulsars", "XMM-Newton", "xray domain", "low msp values", "energy emission", "XMM", "energy emission origin" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Natalie Webb, 2008, 'Why are millisecond pulsar magnetic fields low and how do their X-rays arise', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xgy81xz |