University of Hertfordshire

By the same authors

Hydrodynamic Simulations of Light Bipolar Large Scale Jets

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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Original languageEnglish
Title of host publicationActive Galactic Nuclei: from Central Engine to Host Galaxy, meeting held in Meudon, France, July 23-27, 2002, Eds.: S. Collin, F. Combes and I. Shlosman. To be published in ASP Conference Series, p. 42.
Volume290
Publication statusPublished - 1 Jul 2002
EventAstronomical Society of the Pacific Conference : Active Galactic Nuclei: from Central Engine to Host Galaxy - Meudon, France
Duration: 23 Jul 200227 Jul 2002

Conference

ConferenceAstronomical Society of the Pacific Conference
CountryFrance
CityMeudon
Period23/07/0227/07/02

Abstract

We present new multiwavelength observations of the dwarf Seyfert 1 galaxy POX 52 in order to investigate the properties of the host galaxy and the active nucleus and to examine the mass of its black hole, previously estimated to be ~105 M☉. HST ACS HRC images show that the host galaxy has a dwarf elliptical morphology (MI = − 18.4 mag, Sérsic index n = 4.3) with no detected disk component or spiral structure, confirming previous results from ground-based imaging. X-ray observations from both Chandra and XMM-Newton show strong (factor of 2) variability over timescales as short as 500 s, as well as a dramatic decrease in the absorbing column density over a 9 month period. We attribute this change to a partial covering absorber, with a 94% covering fraction and NH = 58+ 8.4−9.2 × 1021 cm −2, that moved out of the line of sight in between the XMM-Newton and Chandra observations. Combining these data with observations from the VLA, Spitzer, and archival data from 2MASS and GALEX, we examine the SED of the active nucleus. Its shape is broadly similar to typical radio-quiet quasar SEDs, despite the very low bolometric luminosity of Lbol = 1.3 × 1043 ergs s−1. Finally, we compare black hole mass estimators, including methods based on X-ray variability, and optical scaling relations using the broad Hβ line width and AGN continuum luminosity, finding a range of black hole mass from all methods to be MBH = (2.2–4.2) × 105 M☉, with an Eddington ratio of Lbol/LEdd ≈ 0.2–0.5.

ID: 10547383