A dataset provided by the European Space Agency

Name 040092
Title Spectral analysis of the jet in the Seyfert 2 Galaxy NGC 6217 with XMM-Newton
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400920101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400920201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400920301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400920401

DOI 10.5270/esa-2kpnsi5
Author Dr Wolfgang Pietsch
Description The nuclear starburst, flat spectrum spiral NGC6217 offers the possibility to resolve spectrally with XMM-Newton its one-sided jet-like radio and X-ray filament, extending out to 2.7. (18.8 kpc) in the SW of the galaxy. According to ROSAT observations, the jet.s X-ray spectrum seems to be harder than that of NGC6217 and its luminosity in the 0.5-2.0 keV band ~1.7 10E39 erg-s. NGC6217 stands out as the fourth nearest jet galaxy known. Here, we propose a deep XMM-Newton observation of this extraordinary source to resolve the jet from the emission of the galaxy and do a detailed spectral investigation of the jet.
Publication Hard X-ray Emission Associated with White Dwarfs. III. . Bilikova, Jana, Chu, You-Hua, et all. . AJ . 140-1433 . 2010 . 2010AJ....140.1433B ,
The X-ray spectral properties of the AGN population in the XMM-Newton bright serendipitous survey . Corral, A., Della Ceca, R., et all. . A&A . 530-42 . 2011 . 2011A&A...530A..42C ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Fe Kalpha line profile in AGNs: average shape and redshift dependence . Mao, Wei-Ming, Hu, Chen, et all. . RAA . 10-905 . 2010 . 2010RAA....10..905M ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
A systematic cross-search for...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-02-15T16:02:50Z/2007-02-18T05:39:13Z
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 2008-04-13T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-04-13T00:00:00Z, 040092, 17.56_20190403_1200. https://doi.org/10.5270/esa-2kpnsi5