Modelling the orientation of accretion disks in quasars using H-alpha emission
Infrared spectroscopy of the H-alpha emission lines of a sub-sample of 19 high-redshift (0.8 < z < 2.3) Molonglo quasars, selected at 408 MHz, is presented. These emission lines are fitted with composite models of broad and narrow emission, which include combinations of classical broad...
Main Authors: | Down, E, Rawlings, S, Sivia, D, Baker, J |
---|---|
Format: | Journal article |
Language: | English |
Published: |
2009
|
Similar Items
-
Zooming in on quasar accretion disks using chromatic microlensing
by: Blackburne, Jeffrey A
Published: (2011) -
Sizes and Temperature Profiles of Quasar Accretion Disks from Chromatic Microlensing
by: Blackburne, Jeffrey A., et al.
Published: (2012) -
THE REDDENED QUASAR 3C-22 AND ITS IMPLICATIONS
by: Rawlings, S, et al.
Published: (1995) -
Accretion and star formation in quasars
by: White, S
Published: (2015) -
FORGE’d in FIRE II: The Formation of Magnetically-Dominated Quasar Accretion Disks from Cosmological Initial Conditions
by: Philip F. Hopkins, et al.
Published: (2024-03-01)