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The Mass of the Black Hole in the Seyfert 1 Galaxy NGC 4593 from Reverberation Mapping
Author(s) -
K. D. Denney,
Misty C. Bentz,
B. M. Peterson,
Richard W. Pogge,
Edward M. Cackett,
M. Dietrich,
Jeffrey K. J. Fogel,
Himel Ghosh,
K. Horne,
Charles A. Kuehn,
Takeo Minezaki,
Christopher A. Onken,
V. I. Pronik,
D. O. Richstone,
С. Г. Сергеев,
M. Vestergaard,
Matthew G. Walker,
Yuzuru Yoshii
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/508533
Subject(s) - physics , astrophysics , reverberation mapping , galaxy , light curve , black hole (networking) , observatory , line (geometry) , reverberation , emission spectrum , supermassive black hole , astronomy , spectral line , geometry , computer network , routing protocol , routing (electronic design automation) , mathematics , computer science , acoustics , link state routing protocol
We present new observations leading to an improved black hole mass estimatefor the Seyfert 1 galaxy NGC 4593 as part of a reverberation-mapping campaignconducted at the MDM Observatory. Cross-correlation analysis of the H_betaemission-line light curve with the optical continuum light curve reveals anemission-line time delay of 3.73 (+-0.75) days. By combining this time delaywith the H_beta line width, we derive a central black hole mass of M_BH =9.8(+-2.1)x10^6 M_sun, an improvement in precision of a factor of several overpast results.

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