The Mass of the Black Hole in the Seyfert 1 Galaxy NGC 4593 from Reverberation Mapping
| dc.creator | Denney, Kelly D. | |
| dc.creator | Bentz, Misty C. | |
| dc.creator | Peterson, Bradley M. | |
| dc.creator | Pogge, Richard W. | |
| dc.creator | Cackett, Edward M. | |
| dc.creator | Dietrich, Matthias | |
| dc.creator | Fogel, Jeffrey K. J. | |
| dc.creator | Ghosh, Himel | |
| dc.creator | Horne, Keith | |
| dc.creator | Kuehn, Charles | |
| dc.creator | Minezaki, Takeo | |
| dc.creator | Onken, Christopher A. | |
| dc.creator | Pronik, Vladimir I. | |
| dc.creator | Richstone, Douglas O. | |
| dc.creator | Sergeev, Sergey G. | |
| dc.creator | Vestergaard, Marianne | |
| dc.creator | Walker, Matthew G. | |
| dc.creator | Yoshii, Yuzuru | |
| dc.date | 2006-08-18 | |
| dc.date.accessioned | 2026-07-07T10:39:49Z | |
| dc.date.available | 2026-07-07T10:39:49Z | |
| dc.description | 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 H_beta emission-line light curve with the optical continuum light curve reveals an emission-line time delay of 3.73 (+-0.75) days. By combining this time delay with 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 over past results. | |
| dc.description | 22 pages, 3 tables, 5 figures, accepted for publication in ApJ | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0608406 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0608406 | |
| dc.identifier | Astrophys.J.653:152-158,2006 | |
| dc.identifier | doi:10.1086/508533 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/181161 | |
| dc.subject | Astrophysics | |
| dc.title | The Mass of the Black Hole in the Seyfert 1 Galaxy NGC 4593 from Reverberation Mapping | |
| dc.type | text |