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Volumn 297, Issue 4, 1998, Pages 990-998
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Are AGN broad emission lines formed by discrete clouds? Analysis of Keck high-resolution spectroscopy of NGC 4151
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Author keywords
Galaxies: active; Galaxies: individual: NGC 4151; Galaxies: Seyfert; Quasars: emission lines
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Indexed keywords
GALAXIES;
SIGNAL TO NOISE RATIO;
SPECTROSCOPIC ANALYSIS;
BROAD LINE REGION;
CROSS-CORRELATION ANALYSIS;
EMISSION LINES;
GALAXIES ACTIVE;
GALAXIES: INDIVIDUAL: NGC 4151;
GALAXY:SEYFERT;
HIGH-RESOLUTION SPECTROSCOPY;
LOWER LIMITS;
QUASARS: EMISSION LINE;
SEYFERT GALAXIES;
ELECTROMAGNETIC WAVE EMISSION;
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EID: 1842790507
PISSN: 00358711
EISSN: None
Source Type: Journal
DOI: 10.1046/j.1365-8711.1998.297004990.x Document Type: Article |
Times cited : (78)
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References (18)
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