Proposal ID | 030453 |
Title | 1E 1207.4-5209: The Puzzling Radio-quiet Pulsar |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304531501 |
DOI | https://doi.org/10.5270/esa-kmolyg7 |
Principal Investigator, PI | Dr George Pavlov |
Abstract | Chandra and XMM observations of 1E 1207.4-5209, the central compact object inthe SNR PKS 1209--51/52, led to the discoveries of its 424 ms spin period andprominent absorption lines in its thermal-like X-ray spectrum, which provided anexciting opportunity to measure the gravitational redshift at the surface of aneutron star. These observations, spread over a 3.5 yr period, have alsorevealed an intriguing nonmonotonous behavior of the spin period. To understandthe nature of this enigmatic object, we propose a series of observations withthe XMM EPIC detectors. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2005-06-22T12:09:26Z/2005-07-31T19:02:55Z |
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 | 2006-09-09T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "1e 1207", "EPIC", "xray spectrum", "spin period", "intriguing nonmonotonous", "supernova remnant", "gravitational redshift", "yr period", "radio quiet pulsar", "XMM", "enigmatic object", "neutron star", "xmm epic detectors", "prominent absorption lines", "central compact object" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr George Pavlov, 2006, '1E 1207.4-5209: The Puzzling Radio-quiet Pulsar', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kmolyg7 |