Proposal ID | 050082 |
Title | Monitoring the 2007 periastron passage of the pulsar-binary system PSR B1259-63 |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0500820601 |
DOI | https://doi.org/10.5270/esa-mdppqxp |
Principal Investigator, PI | Prof Werner Becker |
Abstract | Non-accreting binary systems containing a spin-powered pulsar and a Be-starprovide us with unique opportunities to investigate the interaction between thepulsar and the stellar wind. We propose to monitor the binary system PSRB1259-63 with its companion Be-star SS 2883 during its periastron passage insummer 2007. This XMM-Newton data will enable us to examine the shocked emissionin a window around periastron in detail and to monitor how the spectral behaviorand the flux evolves when PSR B1259-63 passes through periastron. Thisobservations, which require only a modest amount of observing time, togetherwith archival data taken by ASCA and XMM at other orbital angles will finallyconstrain the geometry of the Be-star disk. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2007-07-20T08:36:30Z/2007-08-03T21:26:34Z |
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 | 2008-09-30T00:00:00Z |
Last Update | 2025-08-04 |
Keywords | "XMM", "XMM-Newton", "2007 periastron passage", "periastron passage", "archival data", "accreting binary systems", "star disk", "xmm newton data", "orbital angles", "spin powered pulsar", "shocked emission", "modest amount", "flux evolves", "summer 2007", "star ss 2883", "stellar wind", "psr b1259" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Prof Werner Becker, 2008, 'Monitoring the 2007 periastron passage of the pulsar-binary system PSR B1259-63', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mdppqxp |