What Does the Geometry of the Hβ BLR Depend On?

What Does the Geometry of the Hβ BLR Depend On?

We combine our dynamical modeling black-hole mass measurements from the Lick AGN Monitoring Project 2016 sample with measured cross-correlation time lags and line widths to recover individual scale factors, f , used in traditional reverberation-mapping analyses. We extend our sample by including pri...

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Váldodahkkit: Lizvette Villafaña, Peter R. Williams, Tommaso Treu, Brendon J. Brewer, Aaron J. Barth, Vivian U, Vardha N. Bennert, Hengxiao Guo, Misty C. Bentz, Gabriela Canalizo, Alexei V. Filippenko, Elinor Gates, Michael D. Joner, Matthew A. Malkan, Jong-Hak Woo, Bela Abolfathi, Thomas Bohn, K. Azalee Bostroem, Andrew Brandel, Thomas G. Brink, Sanyum Channa, Maren Cosens, Edward Donohue, Goni Halevi, Carol E. Hood, J. Chuck Horst, Maxime de Kouchkovsky, Benjamin Kuhn, Douglas C. Leonard, Raúl Michel, Melanie Kae B. Olaes, Daeseong Park, Jordan N. Runco, Remington O. Sexton, Isaac Shivvers, Chance L. Spencer, Benjamin E. Stahl, Samantha Stegman, Jonelle L. Walsh, WeiKang Zheng
Materiálatiipa: Artihkal
Giella:English
Almmustuhtton: IOP Publishing 2023-01-01
Ráidu:The Astrophysical Journal
Fáttát:
Active galaxies
Active galactic nuclei
Seyfert galaxies
Reverberation mapping
Supermassive black holes
Liŋkkat:https://doi.org/10.3847/1538-4357/accc84

Interneahtta

https://doi.org/10.3847/1538-4357/accc84

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