Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005mnras.360.1123p&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 360, Issue 3, pp. 1123-1131.
Astronomy and Astrophysics
Astronomy
30
Galaxies: Active, Galaxies: Individual: Mkn 3, Galaxies: Seyfert, X-Rays: Galaxies
Scientific paper
A 100-ks XMM-Newton observation of the nearby Seyfert 2 galaxy Mkn 3 offers a unique opportunity to explore the complexity of its X-ray spectrum. We find the ~3-8 keV continuum to be dominated by reflection from cold matter, with fluorescent K-shell lines detected from Ni, Fe, Ca, Ar, S, Si and Mg. At higher energies an intrinsic power-law continuum, with canonical Seyfert 1 photon index, is seen through a near-Compton-thick cold absorber. A soft excess below ~3 keV is found to be dominated by line emission from an outflow of `warm' gas, photoionized and photoexcited by the intrinsically strong X-ray continuum. Measured blueshifts in the strong Fe Kα and OVII and OVIII emission lines are discussed in terms of the properties of the putative molecular torus and ionized outflow.
Page Kim L.
Pounds Kenneth A.
No associations
LandOfFree
An XMM-Newton observation of Mkn 3 - a Seyfert galaxy just over the edge does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with An XMM-Newton observation of Mkn 3 - a Seyfert galaxy just over the edge, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An XMM-Newton observation of Mkn 3 - a Seyfert galaxy just over the edge will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1818399