New Arguments Supporting the Intrinsic Origin of BAL QSOs: Formation of the Complex Lyα-NV Line Profile.
Abstract
A study is presented to further elucidate the question of whether or not all quasars are affected by the BAL phenomenon. The possibility that observed BAL profiles are formed in spherically symmetric expanding atmospheres is investigated.
- Publication:
-
Mass Outflows from Stars and Galactic Nuclei
- Pub Date:
- 1988
- DOI:
- 10.1007/978-94-009-2941-8_54
- Bibcode:
- 1988ASSL..142..405H
- Keywords:
-
- Line Spectra;
- Lyman Alpha Radiation;
- Quasars;
- Emission Spectra;
- Near Ultraviolet Radiation;
- Turbulence Effects;
- Astrophysics