A dataset provided by the European Space Agency

Name 005754
Title THE EVOLUTION OF CTB109
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057540101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057540201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057540301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057540401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057540601

DOI 10.5270/esa-h126gcz
Author Dr Paul Plucinsky
Description The supernova remnant (SNR) CTB109 presents a unique laboratory for studying the interaction of SNRs with interstellar clouds: one half of the remnant has expanded unimpeded into a low-density medium and the other half has expanded directly into a dense molecular cloud. The nearly ideal viewing geometry allows the two halves to be cleanly separated. The spectrum of the outer shell, the bright interior emission, and the shock-cloud interface will be well characterized by the three proposed 15 ks pointings. We will determine the ionization structure as a function of position behind the shock, as well as measuring the temperature and abundances. Despite being observed by every major X-ray observatory, there still exists much uncertainty in the physical ..
Publication The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
The Long-term Radiative Evolution of Anomalous X-Ray Pulsar 1E 2259+586 After its 2002 Outburst . Zhu, Weiwei, Kaspi, Victoria M., et all. . ApJ . 686-520 . 2008 . 2008ApJ...686..520Z ,
XMM-Newton Observations of the Galactic Supernova Remnant CTB 109 (G109.1-1.0) . Sasaki, Manami, Plucinsky, Paul P., et all. . ApJ . 617-322 . 2004 . 2004ApJ...617..322S ,
A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations . Muno, M. P., Gaensler, B. M., et all. . ApJ . 680-639 . 2008 . 2008ApJ...680..639M ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L , <...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-01-22T15:51:17Z/2002-07-09T18:28:59Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2003-08-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-08-09T00:00:00Z, 005754, 17.56_20190403_1200. https://doi.org/10.5270/esa-h126gcz