Seyfert 2 galaxy NGC 1808

XMM-Newton Observation of the Seyfert 2 galaxy NGC 1808

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Morphology of the X-ray Emission

NGC 1808

• Extended emission

• Ultraluminous point-like X-ray sources

in the central 600 pc

L 2-10 keV

~10 39 erg/s Zezas, 01

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Nuclear X-ray Emission Morphology of the emission • The spectra of the outer regions are similar • A main part of the hard X-ray emission is originated in the nucleus • The nuclear X-ray emission is harder Region 1 Region 2 Region 3 Region 4 r = 16´´ (850 pc) r = 35´´ (1.9 kpc) r = 2´ (6.4 kpc) r = 20´´- 50´´ (1-2.7 kpc)

Morphology of the X-ray Emission NGC 1808 • Extended emission • Ultraluminous point-like X-ray sources in the central 600 pc L 2-10 keV ~10 39 erg/s Zezas, 01

Page 1 and 2: XMM-Newton Observation of the Seyfe
Page 3 and 4: Introduction X-ray Emission Sources
Page 5 and 6: General Properties of NGC 1808 NGC
Page 7: Morphology of the X-ray Emission EP
Page 11 and 12: Spectral Analysis of the X-ray Emis
Page 13 and 14: Results on the Analysis of the X-ra
Page 15 and 16: Analysis of the optical-UV Emission

Seyfert 2 galaxy NGC 1808

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