A dataset provided by the European Space Agency

Proposal ID 011307
Title A spatially resolved spectral study of the North Polar Spur
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113070101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113070901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0113071001
DOI https://doi.org/10.5270/esa-jeu1s6e
Principal Investigator, PI Dr Bernd Aschenbach
Abstract GT- The bright X-ray feature North Polar Spur (NPS) is the result of a supernovaremnant shock interacting with the inner walls of the giant supershell aroundthe Sco-Cen OB association. It has been shown that the shock from a 10^{51} ergexplosion within the Loop I superbubble can heat the dense shell to temperaturesof 3-4 10^6 K, giving rise to the observed X-ray emission. The shock runninginto the density gradient in the wall is rapidly decelerated, and strong cooling can lead to non-equilibrium effects like overionization.. Using EPIC pn, we canstudy emission line ratios in the 0.3 - 2.0 keV range and thus determine theplasma state. Three adjacent 20 ksec observations will cover the steepestgradient in X-ray brightness.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-09-14T07:52:58Z/2002-03-11T03:04:52Z
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 2005-01-01T00:00:00Z
Keywords "steepest gradient", "emission line ratios", "giant supershell", "bright xray", "inner walls", "overionization '.", "equilibrium effects", "dense shell", "epic pn", "north polar spur", "kev range", "resolved spectral", "xray emission", "EPIC", "sco cen ob", "density gradient", "xray brightness", "erg explosion"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Bernd Aschenbach, 2005, 'A spatially resolved spectral study of the North Polar Spur', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jeu1s6e