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The Structure of the BLR in 3C 390.3.
- Source :
- Proceedings of the International Astronomical Union; 08/07/2009, Vol. 5 Issue S267, p126-126, 1p
- Publication Year :
- 2009
-
Abstract
- Velocity-dependent flux ratios of the broad Lyα, Civ, Hβ, and Hα lines are used to investigate conditions in the archetypical displaced BLR peak emitter 3C 390.3. Our results suggest that gas producing the the UV emission lines has a lower density than the higher-velocity gas producing broad disk-like profile and is less flattened. [ABSTRACT FROM PUBLISHER]
Details
- Language :
- English
- ISSN :
- 17439213
- Volume :
- 5
- Issue :
- S267
- Database :
- Complementary Index
- Journal :
- Proceedings of the International Astronomical Union
- Publication Type :
- Academic Journal
- Accession number :
- 57125595
- Full Text :
- https://doi.org/10.1017/S1743921310005879