MONITORING OF ACTIVE GALACTIC NUCLEI .6. THE QUASAR MKN-876

DOI: 
Publication date: 
01/04/1995
Main author: 
ERKENS, U
IAA authors: 
Authors: 
ERKENS, U; WAGNER, SJ; ALLOIN, D; AXON, D; DEBRUYN, AG; CLAVEL, J; GOAD, MR; GONDHALEKAR, P; VANGRONINGEN, E; JACKSON, N; KOLLATSCHNY, W; LAURIKAINEN, E; LAWRENCE, A; MASEGOSA, J; OBRIEN, P; PENSTON, MV; PEREZ, E; PEREZFOURNON, I; ROBINSON, A; ESPINOSA, JMR; STIRPE, GM; TADHUNTER, C; TERLEVICH, R; UNGER, S
Journal: 
ASTRONOMY & ASTROPHYSICS
Publication type: 
Article
Volume: 
296
Pages: 
90-98
Number: 
Abstract: 
We present the results of a 6 month monitoring campaign of Mkn 876, a low luminosity quasar with M(abs) approximate to -24. High resolution spectroscopy and direct imaging in the Johnson filters B, V, R, I was carried out in the first half of 1990. Line and continuum light curves are presented. Mkn 876 showed a decrease of 17% in the continuum over the whole observing period whereas the line flux of H beta and H alpha stayed constant. This implies, that the radius of the Broad Line Region is larger than 6 light months. Coadded spectra of H beta and H alpha are presented which confirm an extreme asymmetry of the line profiles to the red. With respect to much earlier spectra the line profiles changed considerably.
Database: 
WOK
Keywords: 
GALAXIES, INDIVIDUAL, MKN 876; GALAXIES, SEYFERT; QUASARS, GENERAL; LINES, PROFILE