Proposal ID | 050553 |
Title | X-ray investigation of the first gamma-ray emitter associated with a WR star |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505530101 |
DOI | https://doi.org/10.5270/esa-df7hryl |
Principal Investigator, PI | Mr Jean-Christophe Leyder |
Abstract | A systematic search for hard X-ray and soft gamma-ray emission from Wolf-Rayet(WR) stars, performed using the ISGRI imager, led to the detection of WR 115(26-51 keV). This high-energy emission is expected to be produced by non-thermalrelativistic particles, through several possible mechanisms. However, it isstill unknown which of these proposed mechanisms is responsible for the observedemission, and whether the corresponding X-ray emission is of a thermal ornon-thermal origin. Therefore, we propose to observe this first gamma-rayemitter associated with a WR+O system. These observations of WR 115 withXMM-Newton will help to confirm the origin of the emission seen at higherenergies, and to pinpoint the emission mechanisms thanks to a thorough analysis of its X-ray spectrum. |
Publications |
|
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2008-04-10T11:43:50Z/2008-04-11T04:13:48Z |
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 | 2009-06-06T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "x ray investigation", "nonthermal origin", "isgri imager", "wr star", "gamma ray emitter", "systematic search", "xmm newton", "hard xray", "XMM-Newton", "energy emission", "xray emission", "wr 115", "nonthermal relativistic particles", "XMM", "xray spectrum", "thorough analysis" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Mr Jean-Christophe Leyder, 2009, 'X-ray investigation of the first gamma-ray emitter associated with a WR star', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-df7hryl |