Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Luka Č. Popović"'
Publikováno v:
Advances in Space Research. 71:1219-1226
Publikováno v:
Advances in Space Research. 54:1347-1354
Here we present a new method for subtracting the Balmer pseudocontinuum in the UV part of type 1 AGN spectra. We calculate the intensity of the Balmer pseudocontinuum using the prominent Balmer lines in AGN spectra. We apply the model on a sample of
Autor:
Evaggelia Lyratzi, Emmanouel Danezis, Dimitrios Stathopoulos, Luka Č. Popović, A. Antoniou, Milan S. Dimitrijević
Publikováno v:
Advances in Space Research. 54:1308-1318
In this paper, using the Gauss-Rotation model (GR model), we analyse the UV C IV resonance lines in the spectra of 20 Oe-stars of different spectral subtypes, in order to detect the structure of C IV region. We study the presence and behavior of abso
Autor:
Luka Č. Popović, Stefano Ciroi, Dragana Ilic, Piero Rafanelli, Valentina Cracco, G. La Mura, F. Di Mille
Publikováno v:
Advances in Space Research. 54:1362-1374
It is becoming clear that we can define two different types of nearby AGN belonging to the Seyfert 1 class (S1), on the basis of the match of the intensities of their Broad Balmer Lines (BBL) with the Boltzmann Plots (BP). These two types of S1 galax
Autor:
Luka Č. Popović
Publikováno v:
Advances in Space Research. 54:1147