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Proposal ID 067240
Title Probing the Fermi Bubbles with XMM-Newton
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DOI https://doi.org/10.5270/esa-xsg23bo
Principal Investigator, PI Prof Douglas Finkbeiner
Abstract We propose to investigate the spectrum of X-ray emission from the edge of therecently discovered Galactic gamma-ray features known as the Fermi bubbles. Thebubbles extend 50 degrees above and below the Galactic center, with a width ofabout 40 degrees in longitude. These structures could result from a large-scaleaccretion driven outflow on the central black hole, or winds from a nuclearstarburst. ROSAT X-ray maps (bands R6 and R7) show closely related features witha relatively hard spectrum. This spectrum may be thermal bremsstrahlung emissionfrom T~10^7 K gas, or may contain significant line emission. The proposedobservations can distinguish between these two alternatives.
Publications
Instrument RGS1, EPN, RGS2, EMOS1, OM, EMOS2
Temporal Coverage 2011-09-13T08:09:54Z/2012-03-31T00:55:19Z
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 2013-04-17T00:00:00Z
Last Update 2025-01-27
Keywords "galactic gamma ray", "central black hole", "relatively hard spectrum", "xmm newton", "XMM-Newton", "thermal bremsstrahlung emission", "fermi bubbles", "ROSAT", "xray emission", "line emission", "closely related", "XMM", "nuclear starburst", "galactic center"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Douglas Finkbeiner, 2013, 'Probing the Fermi Bubbles with XMM-Newton', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xsg23bo