High Resolution Spectroscopy of the Nuclear Region of NGC1068 with XMM-Newton/RGS

Details High Resolution Spectroscopy of the Nuclear Region of NGC1068 with XMM-Newton/RGS High Resolution Spectroscopy of the Nuclear Region of NGC1068 with XMM-Newton/RGS

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.0105p&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #01.05; Bulletin of the American Astronomical Society, Vol. 32, p.1181

Astronomy and Astrophysics

Astronomy

3

Scientific paper

The soft X-ray spectrum of the innermost regions (r < 30 arcsec) of NGC1068 as observed with the Reflection Grating Spectrometer on XMM/Newton displays a wealth of discrete features. Preliminary analysis of the spectrum indicates that the emission is completely dominated by recombination in cool, X-ray photoionized gas, with a possible contribution from emission following photoexcitation by the obscured central continuum source. We briefly discuss constraints on the properties of the emission line region derived from the spectroscopic analysis.

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