Proposal ID | 040014 |
Title | Monitoring the spectral variability of the isolated neutron star RX J0720.4-3125 |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400140301 |
DOI | https://doi.org/10.5270/esa-rer9ufx |
Principal Investigator, PI | Dr Jacco Vink |
Abstract | RX J0720.4-3125 belongs to a small group radio-quiet isolated neutron stars,whose X-ray spectra consist of a broad absorption feature superimposed on ablackbody continuum. However, it is unique in that it is the only source inwhich time evolution of the absorption feature and thermal component has beenobserved. The origin of the changes is still unclear, but their study is ofgreat potential importance for revealing physical properties of isolated neutronstars. The spectral evolution may be caused by changes in the stars viewingangle, thermal and/or magnetic field distribution. To distinguish between thesepossibilities, we propose to continue monitoring RX J0720.4-3125. This will alsohelp to further constrain the timing properties of this intriguing source. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2006-05-22T04:44:47Z/2006-11-05T17:24:41Z |
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 | 2007-12-05T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "magnetic field distribution", "time evolution", "isolated neutron stars", "spectral evolution", "rx j0720", "thermal component", "xray spectra consist", "3125 belongs", "spectral variability", "revealing physical properties", "intriguing source", "broad absorption", "J0720.4", "potential importance", "blackbody continuum" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Jacco Vink, 2007, 'Monitoring the spectral variability of the isolated neutron star RX J0720.4-3125', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rer9ufx |