Abstract
Broad, double-peaked Balmer emission lines provide dynamical evidence for the presence of an accretion disk feeding a supermassive black hole in the central engines of AGN.
Original language | English (US) |
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Pages (from-to) | 50 |
Number of pages | 1 |
Journal | Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias |
Volume | 32 |
State | Published - 2008 |
All Science Journal Classification (ASJC) codes
- Space and Planetary Science
- Astronomy and Astrophysics