Discovery of an obscured low luminosity active nucleus in the spiral galaxy NGC 4258

Astronomy and Astrophysics – Astronomy

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Absorption Spectra, Active Galactic Nuclei, Seyfert Galaxies, Spiral Galaxies, Luminosity, X Ray Imagery, X Ray Spectra

Scientific paper

The spectra and images of the nearby jet galaxy NGC 4258 (M106) obtained with ASCA indicate presence of several distinct X-ray emission components. The emission above 3 keV is pointlike and coincident in position with the optical nucleus, exhibiting a hard (photon index approximately 1.78) and absorbed NH approximately 1.5 x 1023 cm-2 spectrum. This provides clear evidence that NGC 4258 hosts an obscured active nucleus of low luminosity, about 4 x 1040 ergs s-1 in 2-10 keV after removing the absorption. Iron K-line emission with an equivalent width 0.25 +/- 0.10 keV was detected. The emission below 1 keV is dominated by an extended approximately 4 min thin-thermal component with a temperature approximately 0.5 keV exhibiting atomic emission lines, possibly associated with the jet. There exists a third continuum component with an intermediate spectral hardness, which is brightest at approximately 1 min south-east of the nucleus.

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