Long-term variability of the optical spectra of NGC 4151. I. Light curves and flux correlations

Astronomy and Astrophysics

Volumn 486, Issue 1, 2008, Pages 99-111

  Shapovalova, A I ^a   Popovic L C ^b,c   Collin, S ^d   Burenkov, An ^a   Chavushyan, V H ^e   Bochkarev, N G ^f   Benitez E ^g   Dultzin, D ^g   Kovacevic A ^h   Borisov, N ^a   Carrasco, L ^e   Leon Tavares J ^c,e   Mercado, A ⁱ   Valdes, J R ^e   Vlasuyk, V V ^a   Zhdanova, V E ^a  

^a RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^b Astronomical Observatory   (Serbia)

^c MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

^f MOSCOW STATE UNIVERSITY   (Russian Federation)

^g UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

^h UNIVERSITY OF BELGRADE   (Serbia)

ⁱ Universidad Politecnica de Baja California   (Mexico)

Author keywords

Galaxies: active; Galaxies: individual: NGC 4151

Indexed keywords

EMISSION SPECTROSCOPY; MONITORING; OPTICAL INSTRUMENTS; OPTICAL TELESCOPES; PHOTOGRAPHY; TELESCOPES;

(2+1) DIMENSIONS; CONTINUUM FLUX; EMISSION LINES; FLUX RATIOS; GALACTIC NUCLEUS; HIGH QUALITY (HQ); LIGHT CURVES; LINE PROFILES; LONG TERM VARIABILITY; OPTICAL CONTINUUM; OPTICAL SPECTRUM; POSITION ANGLE; SPECTRA (CO); SPECTRAL RANGES; SPECTRAL TYPES; TIME LAGS;

FLUXES;

EID: 46649104277     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079111     Document Type: Article

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