Proposal ID | 020393 |
Title | ORIGIN OF THE X-RAY EMISSION OF THE GALACTIC CENTRE MOLECULAR CLOUD SGR B2 |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203930101 |
DOI | https://doi.org/10.5270/esa-8w81lmh |
Principal Investigator, PI | Dr ANNE DECOURCHELLE |
Abstract | We propose a 40 ks XMM-Newton observation of the molecular cloud Sgr B2 locatedin the Galactic Centre. Our aims are to map and characterize both the iron Kline emission at 6.4 keV (line energy and linewidth) as well as its associatedcontinuum (intensity and shape) to determine the nature of this emission:fluorescence due to irradiation by hard X-rays of molecular clouds orinteraction of suprathermal electrons with the molecular gas and/or with the hotplasma at cloud boundaries ? This is a key issue for understanding the highenergy diffuse emission from the Galactic Centre and Sgr B2 is the best locationto carry out this study, as it exhibits the brightest 6.4 keV iron K lineemission in the Galactic Centre, and the weakest diffuse thermal line emission. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2004-09-04T02:52:56Z/2004-09-04T17:01:34Z |
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 | 2005-09-26T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "energy diffuse emission", "kev iron", "galactic centre", "hard xray", "xmm newton", "continuum intensity", "XMM-Newton", "suprathermal electrons", "molecular gas", "hot plasma", "xray emission", "line emission", "XMM", "molecular clouds", "cloud boundaries", "kev line energy", "key issue", "sgr b2" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr ANNE DECOURCHELLE, 2005, 'ORIGIN OF THE X-RAY EMISSION OF THE GALACTIC CENTRE MOLECULAR CLOUD SGR B2', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8w81lmh |