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The Mass of the Black Hole in the Seyfert 1 Galaxy NGC 4593 from Reverberation Mapping

2006/08/18 by Kelly D. Denney, K. D. Denney, Misty C. Bentz +24 · 5 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Astrophysics #Black hole (networking) #Emission spectrum #Galaxies: Formation, Evolution, Phenomena #Galaxy #Geometry #Light curve #Line (geometry) #Observatory #Physics #Reverberation #Reverberation mapping #Spectral line #Supermassive black hole #astro-ph

paper · pdf · doi:10.1086/508533

published as Astrophys.J.653:152-158,2006 · 22 pages, 3 tables, 5 figures, accepted for publication in ApJ

arxiv created 2006/08/18 · openalex publication_date 2006/12/05 · arxiv updated 2009/12/01 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/05

Abstract

We present new observations leading to an improved black hole mass estimate for the Seyfert 1 galaxy NGC 4593 as part of a reverberation-mapping campaign conducted at the MDM Observatory. Cross-correlation analysis of the Hβ emission-line light curve with the optical continuum light curve reveals an emission-line time delay of τ cent = 3.73 ± 0.75 days. By combining this time delay with the Hβ line width, we derive a central black hole mass of M BH = (9.8 ± 2.1) × 10 6 M ☉ , an improvement in precision of a factor of several over past results.

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