X-ray Spectroscopy of Low-Luminosity Active Galactic Nuclei with XMM

Details X-ray Spectroscopy of Low-Luminosity Active Galactic Nuclei with XMM X-ray Spectroscopy of Low-Luminosity Active Galactic Nuclei with XMM

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002stin...0266137d&link_type=abstract

Technical Report, Harvard Coll. Observatory Cambridge, MA United States

Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Astronomical Models, Active Galactic Nuclei, X Ray Spectroscopy, Galaxies, Luminosity, Mathematical Models

Scientific paper

The measurement of black hole masses in nearby galaxies has transformed our understanding of these systems, allowing us to quantify the relevant scales of power, length and time and explore how the activity of black holes is linked to their environments and to the evolution of their host galaxies. In this project, Dr. Tiziana Di Matteo has the primary responsibility for developing and investigating theoretical models for the origin of the X-ray emission observed in low-luminosity AGN. Dr. Di Matteo has been involved in interpreting X-ray data and assessing accretion models throughout the project.

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