LINE SPECTRA; LYMAN ALPHA RADIATION; QUASARS; EMISSION SPECTRA; NEAR ULTRAVIOLET RADIATION; TURBULENCE EFFECTS
Abstract :
[en] 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.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Hutsemekers, Damien ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)
Surdej, Jean ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)
Language :
English
Title :
New arguments supporting the intrinsic origin of BAL QSOs - Formation of the complex Ly-alpha+NV line profile
Publication date :
1988
Event name :
"Mass outflows from stars and galactic nuclei"; Second Torino Workshop
Event place :
Turin, Italy
Event date :
May 4-8, 1987
By request :
Yes
Audience :
International
Main work title :
Proceedings of the Second Torino Workshop "Mass Outflows from Stars and Galactic Nuclei"
